The galaxy presents as a fairly smooth, elliptical morphology with a concentrated central bulge. There's little evidence of distinct spiral arm structure or prominent dust lanes. The color gradient appears to transition from a yellowish hue at the core to a slightly bluer tint towards the outer regions, suggesting some ongoing, albeit limited, star formation activity is occurring. It is predominantly elliptical in shape but displays a slight elongation. The overall structure indicates the possibility of an older stellar population dominating, with a mass estimated in the range of 10^10 to 10^11 solar masses. There are no obvious signs of major mergers or tidal disturbances, though a minor interaction cannot be completely ruled out based on the slight asymmetry.
