The galaxy presents as a relatively smooth, elliptical-like structure, with a centrally concentrated luminosity profile. The core region appears bright and intensely luminous, potentially indicative of a dense stellar population or active galactic nucleus. Moving outwards from the center, the luminosity gradually decreases, forming a diffuse halo surrounding the core. There is little evidence of spiral arm structures or prominent dust lanes. The color profile is consistent with a population of older stars, exhibiting a reddish hue in the outer regions and a bluer tint towards the center. There is no visual sign of a major ongoing merger event.
