The galaxy appears to be a relatively smooth, centrally concentrated object. The primary component exhibits a diffuse, elliptical morphology, with a relatively uniform distribution of light across its surface. There is a secondary, fainter component slightly offset, possibly indicative of a minor interaction or tidal disturbance. Overall, the galaxy appears to be primarily smooth, with a fraction of disk-like features. The colors suggest the presence of a population of older stars, possibly with ongoing star formation. The overall structure is not indicative of a major ongoing merger, suggesting a relatively quiescent state.
