The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. The central region exhibits a bright, concentrated core, indicating a higher density of stars. The isophotes appear elongated, with a moderate flattening. There is a subtle color gradient visible, with the central regions appearing slightly yellower compared to the outer regions, suggesting a population of older stars concentrated towards the core. The galaxy does not show any obvious signs of spiral arm structure or prominent dust lanes. There is some indication of minor asymmetry in the outer regions, potentially suggesting a past or ongoing minor interaction. Overall, it appears to be a relatively evolved, quiescent galaxy with a fairly regular structure.
