The galaxy presents as a single, well-defined object with a generally elliptical morphology, appearing mostly smooth in structure. The primary color observed is a yellow-orange hue, concentrated most intensely towards the galactic center, which transitions outward to a somewhat greener periphery. This color gradient suggests a possible variation in stellar population density and/or age, with the core potentially being dominated by older, redder stars. The relative smoothness and color suggests that this galaxy is an elliptical. No distinct spiral arms or prominent dust lanes are visible in the image. There is no apparent interaction or signs of merger activity present. It seems to be a well formed, solitary galaxy.
