The galaxy presents as a largely smooth, centrally concentrated object. The central region exhibits a yellowish-white hue, suggesting a population of older stars. Diffuse, bluer light extends outward from the central region, possibly indicative of ongoing star formation within a disk. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal features. The overall shape is elliptical, with the roundness exhibiting a slightly in-between state. A faint hint of spiral structure is not inconsistent with the data, though the image resolution is low. Minor irregularities are present in the outer regions.
