The galaxy presents as a slightly elongated, concentrated object with a smooth, featureless appearance. The core exhibits a bright, yellowish-white luminosity, suggesting a significant population of older stars. The overall color profile indicates a lack of substantial ongoing star formation. The galaxy appears relatively undisturbed, lacking any obvious signs of recent mergers or major tidal interactions. The light distribution falls off gradually from the center, with a relatively high Sersic index, indicative of a bulge-dominated morphology.
