The galaxy presents as a somewhat elongated, elliptical shape. The light distribution appears relatively smooth and concentrated towards the center, exhibiting a prominent bulge. The color profile suggests a population of older stars, with a redder hue dominating the central regions and a slightly bluer tint in the outer regions, possibly indicating some ongoing star formation. There is no evidence of spiral arms or a disk-like structure. No tidal tails or significant morphological disturbances are observed, which is consistent with a galaxy that is not currently undergoing a major merger event. The galaxy appears relatively isolated in the field.
