The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its overall shape appears somewhat elliptical, trending towards round rather than elongated. The core region exhibits a yellowish-orange hue, possibly indicating an older stellar population, characteristic of minimal star formation. There is faint evidence of a surrounding envelope or halo, though its extent is difficult to discern due to the image quality. No distinct spiral arms or bar structures are readily apparent. Faint blue regions are observed around the core region of the galaxy, potentially indicative of pockets of star formation. The structure doesn't exhibit obvious signs of major mergers or tidal disruptions, though a minor asymmetry cannot be ruled out.
