The galaxy presents as a lenticular or possibly an elliptical galaxy, elongated in shape. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population. There is a hint of a disk, appearing somewhat diffuse. The outer regions fade gradually, showing a smooth light distribution with no distinct spiral arm structures visible. Overall, the galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions. The galaxy's light profile suggests that it is likely a fairly massive system. Star formation activity appears subdued, indicating a relatively low specific star formation rate.
