The galaxy presents as a centrally concentrated object with a relatively smooth morphology. Its overall color profile suggests a mix of stellar populations. The central region exhibits a yellowish hue, potentially indicative of older, lower-mass stars. A slight bluish tint surrounds the central core, hinting at the presence of younger, hotter stars and possible ongoing star formation activity. The galaxy appears largely undisturbed, with no obvious signs of tidal interactions or major mergers. The overall shape seems close to elliptical, with a moderate degree of roundness.
