The galaxy presents a generally smooth appearance, suggesting an elliptical morphology or a spiral galaxy seen face-on with a dominant bulge. The color profile indicates a predominantly older stellar population, with a yellowish-orange hue dominating the central region. There is a slight elongation, deviating from a perfectly circular shape, with an intermediate roundness. Some faint features are potentially indicative of minor disturbances or asymmetries within the galactic structure. There are no clear signs of major mergers or significant tidal interactions; it appears relatively isolated in its current state.