The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse appearance. The core is a bright, yellow-ish hue, suggesting a population of older stars. There is a color gradient visible from the core outwards, the galaxy appears redder around the edges compared to the yellow center, which could be due to dust absorption or differences in stellar populations. The object is fairly symmetrical, and there are no apparent tidal features or major disturbances indicative of recent major merger events. There's a subtle extension or halo of diffuse light surrounding the central region, further indicating that this is most likely a galaxy with a large halo of older stars. The overall morphology suggests a mature system that is not actively forming stars at a high rate.
