The galaxy appears to be of an elliptical morphology, exhibiting a smooth, concentrated light profile without distinct spiral arms or a prominent disk structure. It demonstrates a moderate degree of ellipticity, appearing somewhat flattened rather than perfectly spherical. The galaxy's color suggests an older stellar population, dominated by redder wavelengths, and a lack of significant recent star formation. It exhibits a bright central bulge with gradually decreasing luminosity towards the outer regions. There are hints of a slight disturbance in the outer structure, which may be indicative of minor past interactions or a merger event. There appears to be a companion galaxy close by.