The galaxy presents as an elliptical or lenticular type, with a smooth, concentrated central bulge that dominates its structure. The overall color profile exhibits a yellowish-red hue, suggestive of an older stellar population. The main body of the galaxy appears well-defined, but without any apparent spiral arms or prominent dust lanes. It exhibits a slight elongation, with the ratio of the major to minor axis indicating it is not perfectly spherical. The outer regions of the galaxy gradually fade into the background sky, without any abrupt truncation. The galaxy does not appear to show any signs of recent major mergers or tidal disturbances. The morphology is consistent with a galaxy undergoing relatively low levels of star formation.
