The galaxy presents as a centrally concentrated, smooth object. The light profile is dominated by a bright, nearly circular core, with a gradual decrease in intensity towards the outer regions. There is some indication of faint extensions or a slight asymmetry in the outer regions. The overall color is a yellowish-orange hue, which suggests an older stellar population. No distinct spiral arm structure or prominent dust lanes are apparent. There do not appear to be any indications of recent major mergers or significant tidal disturbances. Based on these characteristics, the galaxy appears to be an elliptical galaxy, though the possibility of a lenticular galaxy cannot be excluded.
