The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a nearly circular morphology, with a bright, unresolved core region that suggests a significant concentration of older stars. The overall color profile is slightly yellow-white, with faint, diffuse blue emissions extending from the central core. This may indicate a low level of recent star formation in the outer regions, although it is mostly composed of evolved stars. There is little to no evidence of spiral arms or bar structures, nor any prominent dust lanes. The galaxy does not appear to be undergoing any major mergers or tidal disturbances. The apparent smoothness and color profile are suggestive of an elliptical or lenticular galaxy type.
