The galaxy appears to be an elliptical-type, characterized by a generally smooth and rounded morphology. A prominent, bright central bulge is evident, exhibiting a yellowish-orange hue. This likely indicates a population of older, redder stars. The overall distribution of light is relatively even, without strong evidence of spiral arm structures. There appears to be some disruption to the shape of the central bulge which indicates a past or ongoing merging event. There are some regions where the galaxy becomes fainter, indicating a possible tail or extended halo of stars.
