The galaxy presents as an elliptical morphology, exhibiting a smooth, centralized light distribution. The core region appears brighter and more concentrated than the outer regions, with a gradual decrease in luminosity outwards. The galaxy's overall shape is elongated, showing a moderate ellipticity. Color gradients suggest a mixture of stellar populations, with the central regions displaying a slightly yellower hue, possibly indicating a dominance of older, redder stars. Fainter, bluer colors are visible in the outskirts which might correspond to some active star formation. There is no obvious presence of spiral arms or distinct dust lanes within the galaxy. No signs of major mergers or interactions are apparent in the immediate vicinity of the galaxy, though some minor disturbances cannot be ruled out.
