The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light profile appears to decline gradually from the core outwards, showing no distinct spiral arm structures or prominent dust lanes. There is a subtle elongation to the galaxy's shape, although it appears mostly round. Color gradients are subtle, with a slightly bluer tint in the outer regions compared to the more yellow central bulge, potentially indicating some ongoing star formation, albeit at a low rate. The galaxy does not show signs of major mergers or significant tidal disturbances. It is a relatively compact object with a smooth appearance overall.
