The galaxy presents as a generally smooth, centrally concentrated structure. Its overall color appears slightly reddish, suggesting a population dominated by older stars. The galaxy exhibits an approximately elliptical morphology, with a fairly high degree of roundness; it lacks any distinct spiral arm features or a well-defined disk. There is no strong evidence of a recent or ongoing major merger event based on visible tidal tails or significantly distorted morphology, though there may be minor irregularities.
