The galaxy presents as an elliptical or lenticular system, appearing relatively smooth in texture. There is a prominent central bulge, concentrated and luminous, exhibiting a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy, while fainter, indicate a more diffuse structure with a subtle disk-like morphology, elongated along its major axis. The lack of distinct spiral arms or prominent dust lanes supports classification as an early-type galaxy. Overall, the galaxy appears to be fairly isolated, showing no significant signs of tidal disruption or interaction with neighboring galaxies.
