The galaxy presents as a relatively compact object, exhibiting a centrally concentrated light profile. The core region is bright and unresolved, emitting strongly across the observed g, r, and z bands. The overall morphology suggests a generally smooth distribution of light, though subtle features, potentially indicative of minor disturbances, may be present in the outer regions. There is a suggestion of a disk structure, but it's difficult to conclusively discern it from the data provided. The galaxy's estimated size is relatively small, and its overall brightness indicates that it is a mid-range luminosity object.