The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile with a slight elongation. The light is dominated by redder wavelengths, suggesting an older stellar population with low current star formation. There are no apparent spiral arms or disk-like structures. No significant dust lanes or tidal features are visible. The object appears relatively undisturbed and likely not undergoing a major merger. There may be a slight asymmetry or disturbance present.
