The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The light distribution is centrally peaked, fading gradually toward the edges. The galaxy exhibits a yellow hue, indicative of an older stellar population dominating the light output. There is a lack of discernible spiral arm structure or distinct features suggestive of active star formation. The overall shape appears close to circular, with minimal elongation. There is no obvious sign of tidal disturbances or ongoing merger activity. 
