The galaxy presents as a somewhat elliptical, relatively compact structure with a bright, concentrated core region. There is a noticeable falloff in brightness from the center outwards, suggesting a higher density of stars and/or gas in the central region. The galaxy's overall color appears to be a yellowish-white, possibly indicating a population of older stars, though the presence of some bluer regions cannot be excluded given the image quality. The galaxy exhibits a smooth, regular morphology with no obvious signs of strong disturbances such as tidal tails or irregular features, implying that it may not be actively undergoing a major merger event. A hint of an extended, fainter halo may be present, but this is difficult to confirm given the image's resolution. The lack of prominent dust lanes or spiral arm structures further supports the assessment that this system is likely a relatively undisturbed elliptical galaxy.
