The galaxy presents as a roughly elliptical, somewhat flattened structure. Its core exhibits a high degree of brightness, characterized by a concentrated emission profile. Surrounding this core is a more diffuse halo of light, fading gradually outward. There is little indication of distinct spiral arms or prominent dust lanes in the visible light spectrum. Overall, the galaxy appears relatively smooth in texture, with minimal signs of significant ongoing mergers or major tidal disturbances. It seems to be more or less isolated in this frame, as there are no visible nearby companions or indications of any interactions with them. The red-green-blue color distribution suggests that this galaxy is likely a mature system, with a relatively low star-formation rate.
