The galaxy presents as a relatively smooth, elliptical structure with a concentrated central region. The color profile suggests a population of older stars, indicated by the somewhat redder hue compared to actively star-forming galaxies. There is a subtle blue component, concentrated toward the outer regions, which may indicate some ongoing, but relatively low, level of star formation. The galaxy appears largely undisturbed, exhibiting no obvious signs of tidal interactions or major mergers. It shows a generally rounded shape with slight elongation in one axis.
