The galaxy presents as a centrally concentrated elliptical, with a smooth and largely featureless appearance. Its overall color is yellowish-white, indicating a population of older stars. The luminosity is concentrated towards the core, with a gradual decline in surface brightness towards the outer edges, forming a diffuse halo. The galaxy exhibits a slight elongation, deviating subtly from a perfectly circular shape. There is little evidence of ongoing star formation or significant dust lanes within the galaxy, consistent with an evolved stellar population. Faint, asymmetrical disturbances are visible in the outer regions of the galaxy, potentially indicative of a minor past merger event, but this is uncertain. The image suggests a massive galaxy, likely located at a significant cosmological distance.
