The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness outward from the core. The overall color appears somewhat redder, suggesting a population of older stars and a potentially lower rate of ongoing star formation. There is a slight indication of a disk structure but the overall features are smooth. There are no obvious signs of recent or ongoing major merger activity. The galaxy appears to be relatively isolated in its environment.
