The galaxy exhibits a primarily smooth morphology, with a notable lack of defined spiral arms or prominent dust lanes. It appears elliptical in shape, elongated along a major axis. The central bulge is bright and concentrated, displaying a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy are less luminous, with a bluer color, potentially indicating the presence of some younger, hotter stars or low-level star formation. There is a possible minor disturbance or companion galaxy located off to the side, but this feature does not appear to be actively merging with the primary galaxy based on the lack of substantial tidal distortion. The overall structure suggests a relatively evolved system, potentially undergoing a transition to a more quiescent state.
