The galaxy presents a generally smooth, elliptical morphology. Its overall color appears to be reddish, indicating an older stellar population and lower rate of star formation. There is an apparent double nucleus or core, suggesting the possibility of an ongoing or recent merger event between two galaxies. The galaxy exhibits a concentrated central region with diffuse outer edges, and it has an estimated diameter of ~8.5 kpc. There is no clear evidence of spiral arms or prominent dust lanes, and only minor disturbance is apparent, if any.
