This galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a morphology with a dominant bulge component. There is a slight elongation, indicating it is not perfectly spherical, but rather somewhere in between an elliptical and a more elongated shape. There appears to be some minor disturbance in the galaxy's form, possibly indicative of a previous interaction or merger event, or ongoing internal processes that cause some irregularities in its overall structure. The lack of a clear spiral arm structure and the dominant smooth component suggests it is likely a fairly evolved system. The color distribution appears relatively uniform across the galaxy.