The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth appearance and a noticeable radial gradient in surface brightness. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The color transitions outward to a slightly redder tone, maintaining its smooth morphology. There is no clear evidence of spiral arms, dust lanes, or other distinct features that would typically be associated with disk galaxies. The galaxy appears relatively undisturbed, lacking any obvious signs of recent merger activity or tidal interactions.
