The galaxy exhibits a generally elliptical morphology, though with some noticeable asymmetry. It appears to be relatively smooth in overall texture, lacking prominent spiral arms or distinct clumps of star formation regions. The central region of the galaxy shows a concentration of light, suggesting a possible bulge or core. The light profile seems to fade gradually from the center outwards. The object displays a color gradient, with the central region appearing more yellow-orange and the outer regions exhibiting a bluer hue. This color variation may indicate differences in stellar populations, with older, redder stars concentrated in the core and younger, bluer stars more prevalent in the outer regions. There's a subtle hint of a possible tidal feature, with the galaxy appearing slightly disturbed on one side, which might be indicative of a past interaction or merger event, though no significant merger is currently in progress.
