The galaxy presents a somewhat irregular morphology. Its overall light distribution suggests a system that is neither purely elliptical nor a well-defined spiral. There appears to be a relatively bright, concentrated central bulge, which is slightly elongated and not perfectly spherical. The surrounding disk-like structure exhibits hints of spiral arms, although they are not sharply defined or symmetrical.

The color profile indicates a mix of stellar populations. The central bulge shows a yellowish-orange hue, indicative of older, redder stars. Patches of bluer light are visible in the disk region, suggesting the presence of younger, hotter stars and possible ongoing star formation, albeit at a modest rate.

There is evidence of some form of gravitational interaction or disturbance. This is based on the lumpy, somewhat asymmetrical appearance of the disk and potential tidal features extending from the main body. These features suggest that the galaxy may have undergone, or is currently undergoing, a minor merger or close encounter with another galaxy, although no clear companion galaxy is immediately visible in the immediate vicinity within the image. There may also be dust lanes present, obscuring some of the light from behind.
