The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The core exhibits a yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, there's a subtle shift to a more bluish color in the outer regions, implying the presence of some younger, hotter stars. The overall shape is somewhat elliptical, appearing more "in between" than perfectly round. There is no apparent evidence of major mergers or significant tidal disturbances. The structure appears largely undisturbed, with no prominent spiral arms or bar-like features visible. The galaxy likely has ongoing, but not extreme, star formation.
