The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. There are subtle variations in surface brightness, hinting at some internal substructure, though distinct spiral arms or a well-defined disk are not apparent. The galaxy exhibits a radial color gradient, transitioning from a more yellowish hue in the core to a slightly bluer tinge in the outer regions. This suggests a stellar population gradient, with older, redder stars dominating the central bulge and younger, bluer stars populating the outskirts. There is evidence for some minor disturbances in the morphology, potentially resulting from minor interactions, as the outer regions are slightly irregular. However, there are no significant signs of a major merger or tidal disruption. The galaxy is somewhat compact in appearance.
