The galaxy presents as a somewhat elliptical, though not perfectly round, structure. It displays a prominent central bulge that appears bright and yellowish, suggesting an older stellar population dominating the core region. A fainter, bluer halo surrounds the bulge, indicative of more recent star formation activity. The overall smooth appearance suggests it is likely a relatively evolved system. No significant tidal features or strong distortions are apparent, which suggests it has not undergone a recent major merger. However, there are some subtle asymmetries in the outer halo that could be indicative of minor gravitational interactions.
