The galaxy presents as a flattened, disk-like structure with a prominent central bulge. The bulge exhibits a smooth, concentrated light profile, suggesting a high density of older stars. Faint spiral arm structures are possibly present but poorly defined, exhibiting a more flocculent rather than grand design pattern. There's a slight asymmetry in the disk, potentially indicating minor gravitational interaction or internal disturbance. The overall color is slightly redder, which suggests a stellar population dominated by older, less massive stars and potentially significant dust content. Star formation appears to be present, but at a relatively low rate, as evidenced by the lack of bright blue regions. There are no strong indications of a major ongoing merger.
