The galaxy presents as an elliptical structure, exhibiting a smooth morphology with a concentrated central bulge. The color profile suggests an older stellar population, based on the subtle reddish-yellow hue dominating the core and inner regions. The galaxy's shape appears close to round, with a very slight deviation towards an elongated form. There is no strong evidence of recent major merger activity or significant tidal disturbances affecting the galaxy's overall structure. Faint outer regions suggest the presence of a more diffuse halo component. Star formation is likely minimal, indicated by the lack of bright blue regions.
