The galaxy presents as a fairly smooth, elliptical-like structure, with a high degree of central concentration. The galaxy exhibits a bright, compact core that gradually diffuses outward. There is minimal evidence of spiral arm structures or prominent dust lanes. The overall color appears to be on the redder side, suggestive of an older stellar population, with indications of ongoing star formation. The galaxy appears to be quite isolated, showing no immediate signs of tidal interactions or major disturbances. Its overall shape is notably rounded.
