The galaxy presents as a centrally concentrated, relatively smooth structure. Its overall shape appears somewhat elliptical, trending towards being moderately rounded, but not perfectly circular. There is a noticeable color gradient, with the central region exhibiting a yellowish-gold hue, suggesting a population of older stars. The outer regions show a slightly bluer tint, potentially indicating the presence of younger, hotter stars or ongoing star formation. The morphology suggests the galaxy is largely undisturbed, although there may be a minor interaction occurring.
