The galaxy presents as a relatively compact, elliptical-like structure. The overall color profile appears to be redder, possibly indicative of an older stellar population with fewer young, massive stars. There is a smooth, concentrated central bulge, which fades into a more diffuse halo. There appears to be little to no resolved structure such as spiral arms or prominent dust lanes, suggesting the galaxy is likely a relatively undisturbed system. There is some evidence of low-level star formation. There is no evidence of major mergers or interactions.
