The galaxy exhibits an overall elliptical morphology, though some asymmetries are present. The central bulge region is prominent, displaying a smooth, diffuse yellowish color, indicative of an older stellar population. The outer regions show a less concentrated, fainter structure with subtle indications of spiral arms. The color in these outer regions appears slightly bluer than the central bulge, potentially suggesting younger star formation. 

There is a noticeable disturbance or irregularity in the galaxy's shape, with hints of tidal features or minor disturbances present. It may possibly be interacting with a smaller galaxy or experiencing a recent merger event. The relative prominence of the bulge and subtle disk features, combined with the disturbed morphology, suggests a galaxy in transition, possibly evolving from a spiral to an elliptical type through interactions.
