The galaxy presents as a roughly circular, diffuse object. The core exhibits a bright, concentrated luminosity. Surrounding the core is a halo of fainter light extending outwards. There are no obvious spiral arm structures or a distinct galactic disk evident, and the galaxy appears to be relatively smooth in texture. There might be a slight asymmetry in the distribution of light around the core, potentially indicating minor disturbances in the galaxy's morphology. The light profile suggests a relatively concentrated structure, with a smooth decrease in intensity moving outward from the center. There is a central blue hue indicative of the presence of hotter, younger stars residing in the core, with more yellow and red tints around the edge. There is no evidence to immediately suggest an ongoing major merger.
