The galaxy presents as a singular, relatively smooth structure. Its form appears elliptical, displaying a concentrated central bulge that gradually fades outward. The color profile indicates a dominance of older stellar populations, suggesting a subdued rate of star formation. There is no evidence of spiral arms, distinct dust lanes, or active galactic nuclei-related jetting that is apparent in the available imagery. The overall smooth morphology indicates a fairly relaxed system, likely the product of past mergers, or the slow depletion of gas available for star formation.
