The galaxy presents as a moderately sized, relatively smooth object with a roughly elliptical morphology. The central bulge exhibits a concentrated luminosity, appearing significantly brighter than the surrounding disk. A distinct, albeit subtle, color gradient is observed, transitioning from a slightly bluer hue in the outer regions to a yellower tone towards the core. This color variation potentially indicates a younger stellar population residing in the outer disk and an older, redder population dominating the central bulge.

A faint, elongated feature appears to emanate from the central region of the galaxy. It is distinctly bluer, and likely indicates a region of active star formation, perhaps within a distorted tidal arm, or a small companion galaxy that could be the source of minor disturbances within the overall structure of the galaxy. The primary structure appears undisturbed; however the presence of this faint feature indicates minor interactions may have occurred. 
