The galaxy presents as a centrally concentrated structure with an overall smooth appearance. There is a slight elongation of the galaxy along one axis, giving it a somewhat cigar-shaped morphology. The central region displays a brighter, more yellow/gold color, indicative of an older stellar population. The outer regions appear fainter with a slight indication of bluer hues, suggesting the presence of some younger stars, although to a lesser extent than the central region. There are no obvious spiral arm structures or major disturbances, the galaxy's shape does not strongly suggest any ongoing major mergers. Faint color variations hint at possible substructure or minor tidal features, but these are not distinct. The galaxy appears relatively isolated and undisturbed.
