The galaxy presents as a somewhat elliptical morphology, although a slight disk-like structure is suggested. A prominent central bulge is visible, displaying a yellowish hue, potentially indicating a population of older stars. The outer regions exhibit a bluer tint, suggesting ongoing or recent star formation, though this activity appears moderate rather than intense. Overall, the galaxy seems relatively undisturbed with no clear signs of major mergers or significant tidal disruptions. There may be some presence of dust lanes within the galaxy, but resolution is not clear enough to definitively observe them.
