The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a high density of stars. A fainter, more diffuse halo surrounds the core, gradually fading into the background sky. There is a slight elongation, but the galaxy is mostly round. The galaxy exhibits a yellowish-white hue in the core, possibly indicating an older stellar population and minimal dust obscuration. Faint, diffuse blue extensions are visible towards the periphery. The disk may be slightly disturbed, possibly from tidal forces, but it does not show any significant merger activity.
