The galaxy presents as a centrally concentrated object with a smooth, diffuse light distribution. It appears elliptical in shape, with a high degree of roundness. No distinct features such as spiral arms or a prominent disk structure are visible. There are no indications of any major mergers or tidal disturbances. The galaxy exhibits a color profile that is somewhat redder than that of typical spiral galaxies, suggesting an older stellar population and a relatively low rate of ongoing star formation. The object appears to be relatively compact with a moderate apparent size. The overall morphology suggests that it is an early-type galaxy, likely an elliptical or lenticular galaxy at a considerable distance.
