The galaxy presents as a relatively smooth, elliptical-like structure. Its overall color is yellowish-orange, suggesting an older stellar population. The light is centrally concentrated, with a bright core that gradually fades towards the outer edges. There is no apparent spiral structure, nor are there any signs of significant dust lanes or recent star formation regions visible within the galaxy. The galaxy exhibits a high degree of symmetry and circularity, though some slight irregularities are apparent in the outermost fringes of light. These could indicate minor tidal disturbances or interactions with smaller companion galaxies, however no evidence of active merging is evident. The galaxy appears to be relatively isolated in the field, consistent with a possible membership in a low-density group or field environment.
