The galaxy presents as a relatively smooth, centrally concentrated system. It appears roughly elliptical in shape, exhibiting a gradual decline in surface brightness from the core outward. No prominent spiral arms or bar structures are discernible. The overall color appears slightly reddish, suggestive of a population of older stars and a low rate of ongoing star formation. There is no obvious evidence of recent mergers or significant tidal disturbances. It has an apparent moderate size, consistent with a low redshift. The core appears bright and somewhat unresolved.
