The galaxy appears as a centrally concentrated, largely smooth structure. Its color is predominantly yellow-orange, suggesting an older stellar population. The galaxy exhibits an elliptical or spheroidal morphology, lacking any obvious spiral arms or disk-like features. There are no strong signs of recent or ongoing major mergers or tidal disturbances. The light distribution fades gradually from the center outwards, showing a relatively diffuse halo. A slight elongation may be present but without well-defined features, although the galaxy does appear largely round. There are no clear indications of significant dust lanes or star forming regions in the galaxy image.
