The galaxy presents as a luminous, centrally concentrated object with a smooth overall morphology. It appears elliptical, exhibiting a nearly circular shape. The core region displays a bright, yellowish-white hue, indicating a high density of older stellar populations. A gradual color gradient transitions from the core outwards to the edges of the galaxy, exhibiting a slightly bluer tint, hinting at the presence of some younger stars or ongoing star formation, but at a low rate. There is no evidence of spiral arms or a well-defined disk structure. The galaxy lacks prominent features suggestive of recent major merger activity, though a faint asymmetry or minor disturbance cannot be completely ruled out. The galaxy is relatively compact, with a limited spatial extent.
