The galaxy presents as a singular, relatively smooth structure with a generally elliptical morphology. It exhibits a concentrated, bright central region that gradually diffuses outwards into a less luminous halo. The color profile suggests a population of older stars, with a dominant yellowish-red hue in the core transitioning to a slightly bluer tint in the outer regions. There is no apparent spiral structure or distinct dust lanes visible. The overall impression is that of a mature galaxy with limited ongoing star formation.
