The galaxy presents as a centrally concentrated elliptical or lenticular type. Its light distribution is largely smooth, with the highest intensity in the core region, which exhibits a yellowish hue. This suggests an older stellar population concentrated towards the center. The overall shape is somewhat elongated, but not significantly cigar-shaped, with a relatively high degree of symmetry. There is no prominent disk structure visible, nor any indications of spiral arms or significant dust lanes. Faint extensions or tidal features are not readily apparent, suggesting it is not currently undergoing a major merger, but minor disturbances cannot be ruled out. The outer regions display a gradual decrease in luminosity, blending into the background sky. The overall color profile indicates a relatively quiescent galaxy, likely with a low star formation rate.
