The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, lacking any prominent spiral arms or distinct features. The color profile suggests a population of older stars, contributing to the overall yellowish-white hue. There is a slight bluing of the outer edges, which could indicate some ongoing, although subdued, star formation. The galaxy's form exhibits a largely rounded shape. There appear to be no signs of ongoing major mergers or significant tidal disturbances.
