The galaxy presents a generally elliptical morphology, though with some indication of spiral arm structure. The central bulge region appears bright and concentrated. The surrounding disk exhibits a slightly blue hue, potentially indicative of ongoing or recent star formation. There are suggestions of disturbance, potentially caused by minor or major interactions with neighboring galaxies, as evidenced by the irregularity in the shape. The galaxy's structure is not entirely smooth; there are features that hint at a complex history, possibly involving mergers or tidal interactions. The lack of clear dust lanes suggests it may be transitioning towards a more quiescent state. Overall, the galaxy displays properties intermediate between a spiral and an elliptical, exhibiting a morphology characteristic of an intermediate type galaxy in a state of moderate activity.
