The galaxy presents a moderately luminous and concentrated light profile. It appears mostly smooth and elliptical, with no obvious spiral arm structure or bar features visible. The galaxy exhibits a slight elongation. There are no strong signs of ongoing star formation in the form of blue knots or irregular features. Some minor disturbances are possible but not prominent. There appears to be a large fraction of artifact/blur to this image. The light distribution suggests a system dominated by an older stellar population, potentially indicative of a relatively quiescent period of star formation. The estimated size is around 12 kiloparsecs. It could be a moderately massive galaxy, but may be in the process of merging.
