The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light profile appears to gradually decrease from the core outwards. There is a slight elongation noticeable; the galaxy is in between round and cigar shaped. The core appears to be dominated by yellow light, suggesting a population of older stars. A subtle transition to redder hues may be present in the outer regions, with a hint of younger, bluer stars interspersed within the galaxy disk. No spiral arm structures are visible. There are no indications of a major merger or tidal disturbance. There appears to be only minor disturbance.
