The galaxy presents as a relatively compact, moderately luminous object with a smooth, diffuse morphology. It is elliptical, appearing neither perfectly spherical nor highly elongated. The central region exhibits a higher concentration of light, gradually decreasing in intensity towards the outer edges. There is minimal evidence of spiral arm structures or distinct features, suggesting a lack of significant recent star formation. The overall color appears slightly redder than average, which could indicate an older stellar population and a low rate of ongoing star formation. The general form and lack of disruption suggest it may be a relatively undisturbed system that is not currently interacting with another galaxy, although minor tidal features or disturbances may be present but not readily apparent in this imaging. There is a hint of disk-like morphology.
