The galaxy presents as a somewhat amorphous structure, exhibiting a mixed morphology. There is a central bulge, characterized by a concentrated region of intense yellow-white light, suggesting a high density of older stars. Diffuse, fainter regions surround this core, exhibiting bluer hues, which might indicate ongoing star formation. The overall shape is irregular, showing some distortion. Some disruption appears evident, perhaps due to a minor gravitational interaction or a past merger event. The galaxy exhibits characteristics of both a smooth elliptical galaxy and a disk galaxy, lacking defined spiral arms. The galaxy's estimated size is a few kiloparsecs across. Overall, this is likely a galaxy currently undergoing some minor disruption with a moderate amount of ongoing star formation.
