The galaxy presents as a centrally concentrated, elliptical structure. Its overall morphology appears smooth with no apparent spiral arms or other distinct features. The color profile is predominantly yellow, suggesting a stellar population dominated by older stars. The isophotes appear largely round and regular, with no obvious signs of ongoing merger activity or significant tidal disturbances. The galaxy exhibits a relatively compact size, and possesses a high degree of central surface brightness concentration. The outer regions of the galaxy fade gradually into the background, indicating a diffuse halo component. There is no evidence of significant dust lanes or prominent star-forming regions.
