The galaxy presents as an elliptical morphology, with a smooth, centralized concentration of light. A dominant, bright nucleus is visible. Moving outward from the nucleus, the light intensity gradually diminishes. While the galaxy lacks apparent spiral arms, the isophotes show some subtle deviation from a perfectly circular shape, giving the impression of a slight elongation, but is generally quite round in shape. Color gradients are also visible across the face of this system. The central region displays a more yellowish hue, suggestive of an older stellar population. Towards the outer edges, the color shifts slightly to bluer tones, potentially indicating the presence of a younger, more metal-poor stellar population and some low-level star formation activity. There is no obvious sign of strong tidal features or interactions, the galaxy's form looks to be well settled. 
