The galaxy presents as an elliptical or lenticular type. It exhibits a bright, concentrated central bulge that dominates the overall structure. A flattened disk is present, extending outwards from the bulge, though it appears relatively smooth and lacks prominent spiral arm structures. The disk shows evidence of a gradual decrease in luminosity with increasing radial distance from the center.

The galaxy displays a yellow-red color gradient that is strongly concentrated in the center. The outer regions of the galaxy show a more blueish hue, suggesting ongoing star formation. However, overall the galaxy is dominated by older stellar populations. The overall shape suggests minimal interactions, however, there appears to be some minor disturbance in the outer edges of the galaxy. 
