The galaxy presents a generally smooth morphology, appearing primarily elliptical in shape, though there may be some disturbance due to interactions with nearby galaxies. The central region exhibits a bright, concentrated luminosity, suggestive of an older stellar population. The main body of the galaxy shows a yellow-white hue that gradually shifts to a fainter, bluer color in its outer regions. This color gradient might reflect differing stellar populations, with the core being dominated by older, redder stars and the outskirts containing younger, bluer stars. There appears to be evidence of a possible ongoing or recent merger event or some kind of tidal disturbance, as indicated by subtle distortions in the galaxy's overall shape.
