The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical or lenticular in morphology, lacking prominent spiral arm structures. The light distribution is dominated by a bright, centrally located bulge that gradually fades towards the outer regions. A slight elongation is apparent, suggesting it is not perfectly spherical. The color profile shows a yellowish-white hue, indicating an older stellar population, with low to moderate ongoing star formation. Faint disk-like structure may exist but is difficult to discern. There is no evidence of major tidal disturbances or ongoing merger activity. The overall impression is that of a mature, relatively quiescent galaxy.
