The galaxy presents a moderately smooth, disk-like structure with a noticeable central bulge. The disk component displays a faint bluish tinge, possibly indicative of ongoing star formation, particularly in the outer regions. The inner regions appear more yellow, consistent with an older stellar population. The galaxy exhibits a slight ellipticity, appearing more "in between" round and cigar shaped. There is also a subtle suggestion of some minor disturbance to the morphology, although there are no obvious major mergers or tidal tails visible. Overall, the galaxy appears to be a relatively quiescent system, somewhere in the transition between a spiral and an elliptical galaxy.
