The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears largely spheroidal, with a gradual decrease in luminosity outwards. The color profile suggests an older stellar population, evidenced by the reddish-yellow hue concentrated in the bulge, potentially indicative of a low star formation rate. There is some bluer light on the edge of the disk that may be some star formation. The galaxy appears relatively isolated, showing no obvious signs of a major merger event. There is a possibility of a minor disturbance on the disk, but the morphology is largely undisturbed.
