The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical in shape. The overall color profile suggests a population of older stars, with a bias towards redder wavelengths, but there's also evidence of a significant blue component. There is a lack of distinct spiral arm structures or prominent dust lanes. The galaxy does not show any clear signs of ongoing major mergers, although there might be minor disturbances present. The light distribution falls off smoothly from the center outwards, with no sharp boundaries or abrupt changes in brightness.
