This galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears to be largely featureless, suggesting an elliptical morphology, or potentially a spiral galaxy seen face-on with limited visible structure. The central region exhibits a bright, compact core that gradually fades outwards. There is a slight elongation, deviating from a perfectly circular shape, but it is close to round. The color gradient suggests older stellar populations, as indicated by the yellowish hue, in the central bulge. Fainter, bluer light surrounding the bulge suggests the presence of younger stars in the outer regions, but these are less pronounced. There is no strong evidence of spiral arms, dust lanes, or active star formation regions based on this image alone. No major mergers or tidal disturbances are evident, although there is a very minor possible disturbance.
