The galaxy appears as a single, centrally concentrated object. It has a generally elliptical or spheroidal morphology. The light profile is smooth and without obvious spiral arms or a well-defined disk structure. The core exhibits a slightly yellowish hue, which may indicate an older stellar population. The surrounding envelope of the galaxy gradually fades into the background. There are no obvious signs of ongoing merging activity or tidal disturbances. Based on its round shape and the lack of a visible disk, this galaxy is likely an elliptical galaxy.
