The galaxy presents a generally elliptical morphology, though with hints of a disk-like structure. It exhibits a moderately smooth appearance, potentially indicating an older stellar population. There are suggestions of some internal features, such as faint spiral arm structures, or perhaps tidal disturbances. There appears to be a slight asymmetry to the galaxy's shape, with a possible minor distortion on one side. This could indicate a past minor merger event or interaction with a smaller companion. The galaxy's central region is brighter and more concentrated, suggesting a bulge component. The color profile indicates a mix of stellar populations, with hints of both older, redder stars and younger, bluer stars, particularly in the faint disk-like regions. Overall, the galaxy appears to be in a transitional phase, possibly evolving from a more spiral-like structure to a smoother, more elliptical form due to past interactions.
