The galaxy presents as a relatively smooth, elliptical object. Its morphology indicates a likely early-type galaxy, specifically an elliptical galaxy given its ovoid shape. It does not exhibit any prominent spiral arms or a distinct disk structure. There is an apparent nucleus that is bright and compact. Faint evidence of possible minor disturbances can be observed which may suggest that the galaxy could be undergoing a minor merger. The light distribution suggests a moderate concentration towards the center, with a gradual fall-off in luminosity moving outward. The color appears largely uniform, with a slight redder hue in the central region, indicative of an older stellar population.
