The galaxy presents as a single, relatively smooth object. It exhibits a generally elliptical morphology, though some subtle deviations from perfect elliptical symmetry are present. The galaxy's light is concentrated towards the center, with a gradual decrease in brightness observed towards its outer regions. A notable color gradient exists, with a reddish hue dominating the central region, transitioning to a bluer color in the outer regions. This color variation may indicate differing stellar populations, with older, redder stars concentrated in the center and younger, bluer stars residing in the disk. No strong evidence of spiral arm structure or a prominent disk is immediately apparent. There are hints of minor disturbances in its morphology, perhaps a faint tidal feature, but the overall appearance is largely undisturbed.
