The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-white hue, indicative of a population of older stars. The light gradually diminishes outward from the core, transitioning to a fainter, greenish-blue halo. The absence of distinct spiral arms or prominent dust lanes suggests the classification of the galaxy to be either an elliptical, or possibly a lenticular galaxy viewed face-on. There is no obvious evidence of ongoing major mergers, although a subtle asymmetry in the outer regions could possibly indicate a minor tidal interaction or past merger event. The overall roundness of the object and smooth light profile support the notion of a fairly relaxed stellar distribution. The angular size is relatively small, pointing to the galaxy being at a considerable cosmological distance, with its intrinsic physical size calculated to be approximately 7.7 kpc.
