The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a diffuse, rounded morphology with no discernible spiral arms or bar structure. The color gradient suggests a possible presence of an older stellar population, with the central region exhibiting a slightly redder hue, indicative of potentially older stars. The outer regions appear bluer, which may suggest some recent or ongoing low level star formation, but overall it is mostly smooth, lacking prominent features generally associated with ongoing or very recent major star formation events. There is no evidence of significant tidal disturbances or ongoing mergers in this image. The galaxy exhibits a somewhat elliptical shape, as opposed to being perfectly circular.
