The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. The galaxy displays a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a redder color towards the central bulge. There are no obvious spiral arm structures or significant dust lanes visible in this image. The overall morphology suggests a relatively evolved stellar population. Some minor irregularities in the outer halo are present, potentially indicating some sort of gravitational interaction or past merger event.
