The galaxy appears to be a relatively smooth, centrally concentrated object. Its overall shape is elongated, exhibiting a cigar-like morphology, with a ratio of major to minor axes estimated around 3:1. There is a dominant, bright central region which suggests a significant concentration of stars or an active galactic nucleus, although no distinct nucleus is resolved in the image. The color profile suggests a slightly bluer hue in the central regions, transitioning to redder tones in the outer regions. The overall smooth appearance indicates that the galaxy is likely an elliptical or S0 type, but there is some indication of possible tidal features or disturbances in the outer regions, warranting further investigation into potential past merger events, or ongoing minor disturbances.
