The galaxy presents as a single, somewhat diffuse object with a notable central concentration of light. The overall shape appears largely elliptical or spheroidal, exhibiting a smooth profile without prominent spiral arms or a well-defined disk structure. Coloration is primarily yellowish, suggesting an older stellar population. The galaxy's estimated size is a modest fraction of a degree, and there are no obvious signs of strong tidal interactions or recent major mergers, although there are some irregularities visible. These irregularities may be due to a minor disturbance or a past merger event.
