The galaxy appears to be a relatively compact, spheroidal system, possibly an elliptical galaxy or a lenticular galaxy seen at a low inclination. The light profile appears smooth and centrally concentrated with no apparent spiral arm structure or prominent dust lanes. The color is generally yellowish-orange, suggesting an older stellar population, likely dominated by evolved stars. There is a slight color gradient, with the core potentially appearing more yellow than the outer regions, indicating a possible variation in stellar population or metallicity. No strong signs of active star formation are readily apparent from the broad-band imaging. There is no indication of any major disturbances or ongoing mergers with other galaxies in the immediate vicinity.
