The galaxy presents as a somewhat elliptical structure with a concentrated central bulge. It exhibits a smooth overall appearance, lacking prominent spiral arms or other distinct features. The core region is significantly brighter and yellower than the outer regions, suggesting a higher concentration of older stars. The color gradient transitions smoothly from the yellow center to a slightly redder hue in the outer halo. There is minimal evidence of ongoing major star formation, as indicated by the lack of bright blue regions typically associated with young, hot stars. A very slight asymmetry might be present, but the galaxy predominantly appears undisturbed, with no clear signs of recent major mergers or tidal interactions.
