The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. There's a noticeable gradient in luminosity, with the core region appearing significantly brighter and more yellow in color than the surrounding halo. The overall shape approximates a slightly elongated spheroid, with a relatively small physical size. There is no evidence of a prominent disk, spiral arms, or ongoing major merging activity. Subtle color variations exist within the galaxy's structure, with a slight tendency towards bluer hues in the outer regions, potentially indicating the presence of younger stellar populations compared to the core. The galaxy appears to be relatively undisturbed.
