The galaxy presents as a fairly smooth, elliptical structure. It exhibits a somewhat rounded morphology, appearing neither perfectly circular nor highly elongated. There may be a slight indication of a disk. The galaxy's overall color is moderately red, suggesting an older stellar population and reduced recent star formation activity. There is no obvious evidence of any major disturbances or ongoing merger activity. There is little to no indication of spiral arm structure. The galaxy appears relatively isolated in this field of view.
