The galaxy presents as a centrally concentrated object, exhibiting a roughly elliptical morphology. Its core region displays a bright, yellowish hue, indicating a potentially older stellar population. A gradual color gradient is observed moving outwards from the core, transitioning into a more greenish-yellowish halo. The edges of the galaxy appear somewhat diffuse, lacking sharp, well-defined boundaries. There is a slight asymmetry in the overall shape, which may be indicative of minor interactions or internal processes. Evidence of disk-like structure is not readily apparent. Overall, the galaxy gives the visual impression of a relatively quiescent system, potentially in a late stage of its evolution.
