The galaxy presents as a slightly elongated, luminous object with a prominent central bulge. The core region exhibits a yellowish hue, suggesting a population of older stars. Surrounding this central region is a less concentrated disk or halo, displaying a bluer tint indicative of younger, hotter stellar populations or possible ongoing star formation. The galaxy appears relatively undisturbed, without any obvious signs of major mergers or tidal interactions. However, there is a subtle asymmetry in the outer regions which may indicate minor interactions. Overall, the galaxy exhibits a smooth morphology, transitioning from the bright bulge to a less dense outer structure.
