The galaxy presents as a single, centrally concentrated object. It exhibits a largely smooth, elliptical morphology with no apparent spiral arm structure or significant disk component. The light profile suggests a centrally dominant bulge. The color index, inferred from the brightness in different bands, indicates a population of older stars, contributing to its yellowish hue. There are no obvious signs of ongoing major merger activity or tidal disturbances. The general roundness suggests a relaxed dynamic state.
