The galaxy presents a generally smooth, rounded morphology, suggesting a classification as an elliptical or lenticular galaxy. The light is concentrated in the center and becomes more diffuse with radial distance from the center. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy's color is a yellow-red hue, possibly indicating an older stellar population and a relatively low rate of recent star formation. There is the suggestion of a minor tidal interaction or disturbance within the galaxy's halo, which could potentially be indicative of a minor merger event. Overall, the galaxy appears to be relatively undisturbed.