The galaxy presents a generally smooth and elliptical morphology. It exhibits a bright, concentrated core region that appears yellowish in color, suggesting an older stellar population. The isophotes are mostly regular and show only a slight ellipticity, trending towards a more circular shape. There is little to no evidence of spiral arms or significant dust lanes. A faint, diffuse halo surrounds the central region, exhibiting a bluer hue which suggests a sparse population of younger stars. No obvious signs of recent major merger events are observed, though there are indications of minor disturbances to the main structure.
