The galaxy presents as a single, relatively smooth object with a centrally concentrated light profile. It appears nearly circular with a slight elongation. The galaxy's core exhibits a bright, yellowish hue, suggesting a population of older stars. A subtle gradient of color is observed moving outwards, transitioning to a faint greenish tint. There is no evidence of spiral arms or a distinct disk structure. The overall morphology indicates a lack of significant ongoing star formation. No signs of major mergers or tidal disturbances are apparent, suggesting the galaxy is relatively undisturbed.
