The galaxy presents a relatively smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity, suggestive of an older stellar population. There is a slight elongation in the galaxy's shape, and a faint disk appears to be present surrounding the center. Faint wisps of blue light are visible within the halo, indicating some ongoing star formation. The galaxy appears relatively isolated, with no obvious signs of a major merger or significant tidal disturbances. The overall color suggests that the galaxy is comprised of an older stellar population, and appears to be quite massive.
