The galaxy presents a largely smooth, elliptical morphology. It exhibits a central concentration of light that diffuses outwards into a less dense halo. The core appears to have a slightly reddish hue, which may indicate an older stellar population. Faint bluish tinges appear in the surrounding regions of the galaxy which may indicate some regions of younger stars, or it may simply be image artifacts. There's a suggestion of minor asymmetry in the outer regions, perhaps indicative of a past or ongoing interaction, but there are no obvious tidal tails or bridges visible. The overall color indices suggest a system dominated by older stars, though with a low level of recent or ongoing star formation.
