The galaxy presents as a single, relatively smooth object. It exhibits a generally elliptical morphology, appearing largely spheroidal with minimal discernible structure. The light distribution suggests a centrally concentrated spheroid, with a gradual decrease in intensity towards the outer regions. The galaxy's color appears to be dominated by longer wavelengths, indicative of an older stellar population. There appears to be some minor disturbance or merging occurring as there are some asymmetries on the edges of the spheroid. There are no clear signs of strong star formation.
