The galaxy presents a generally smooth and elliptical morphology. The central region exhibits a bright, concentrated core, indicating a possible bulge. The light distribution decreases gradually from the core outwards, fading into a diffuse halo. The overall color appears relatively uniform across the galaxy, trending towards a bluer hue, with slight variations in color across the galaxy, with a few redder regions that may be the results of more dust obscuring the light from the galaxy, or different stellar populations. There is little indication of spiral arm structure. Based on the data, this galaxy likely contains a high amount of older stars, but there are possibly younger star populations also present. There is no evidence of strong tidal disturbances or recent merger activity, though some minor disturbances may be present.