The galaxy presents a generally smooth morphology. It appears mostly elliptical, exhibiting a high degree of central concentration. The galaxy's color suggests a population of older stars, likely dominated by redder spectral types. There is little evidence of spiral arm structure or significant dust lanes. Some minor disturbances or faint features are possible near the periphery, but the primary impression is one of a relatively undisturbed elliptical galaxy. There are no clear indications of ongoing major mergers or strong tidal interactions.