The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge region that is bright, and appears yellow-orange in color. The light profile suggests a relatively evolved stellar population within the bulge. Moving outward from the center, the light gradually diminishes, forming a diffuse halo. There is no discernible spiral arm structure or prominent dust lanes. Overall, the galaxy appears to be an early-type galaxy, likely an elliptical galaxy, with no signs of recent major mergers or tidal disturbances.
