The galaxy presents a primarily smooth, elliptical morphology. The central region exhibits a concentrated luminosity profile, suggesting the presence of an older stellar population. The overall color appears to be slightly redder, consistent with an evolved stellar population and/or the effects of dust extinction. There is a faint, extended halo surrounding the central region, with hints of a disk. No strong tidal features or signs of major mergers are apparent in the image. The galaxy appears relatively undisturbed.
