The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution. Its core appears bright and concentrated, with a color profile tending towards yellow-orange. The outer regions of the galaxy show a bluer hue, possibly indicative of a younger stellar population or ongoing, low-level star formation within the galaxy's disk-like structure. There is no evidence of strong spiral arm structures or prominent dust lanes, suggesting a relatively undisturbed system that hasn't recently experienced a major merger event, but there may be minor disturbances. The galaxy displays a moderate ellipticity, with a shape somewhere between round and elongated. Overall, the galaxy's appearance indicates a system in transition, moving from a more actively star-forming state to a quiescent elliptical galaxy.
