The galaxy presents a largely featureless, elliptical morphology. Its light profile is dominated by a smooth, centrally concentrated bulge exhibiting a yellowish hue. There is very little evidence of spiral arm structure or prominent dust lanes. The galaxy appears relatively round. Minimal structural distortions are discernible, indicating little to no current major merger activity. The overall color suggests a stellar population that is dominated by older stars, with a limited amount of ongoing star formation. It seems to be a relatively massive system.
