The galaxy appears to be a relatively smooth, elliptical type with a concentrated central bulge. It exhibits a nearly circular morphology. There is a subtle color gradient visible, transitioning from a slightly bluer hue in the outer regions to a more yellowish color in the central bulge, indicating a possible difference in stellar populations, with older stars concentrated towards the core. Based on color indices, it is likely in the green valley, as the star formation is slowing or has already been quenched. There is no evidence of spiral arms, bars, or significant dust lanes. Small tidal features could be present, but the resolution is insufficient to confirm. The mass of the galaxy is likely around 10^10 solar masses.
