The galaxy presents as a relatively smooth, centrally concentrated object, with a discernible, though diffuse, halo extending outwards from the central region. The core exhibits a yellowish-white hue, indicative of an older stellar population. There is a marginal suggestion of bluer components in the outer regions, which could be related to patches of younger, star-forming regions, though this is difficult to resolve definitively. There's no apparent spiral structure or strong evidence of a disk. Overall, the morphology suggests an elliptical galaxy, possibly with some ongoing, low-level star formation in its periphery. It does not appear to be undergoing any major merging events, though there is some slight asymmetry in the outer halo which could be evidence of minor disturbances.
