The galaxy presents a disk-like morphology with a central bulge. It appears to be undergoing some form of interaction or disturbance, potentially a minor merger, evidenced by the asymmetrical shape and faint tidal features or distortions extending from the main body. The color distribution suggests ongoing star formation within the galaxy. The central region appears more concentrated and exhibits a brighter, somewhat redder hue, possibly indicating an older stellar population in the bulge. The outer regions display a bluer tint, consistent with the presence of younger, hotter stars in the spiral arms or disk. The overall structure seems somewhat irregular, lacking the defined spiral arm structure. There are no prominent dust lanes visible in this image. The galaxy appears relatively small.
