The galaxy presents as a centrally concentrated object with a smooth, diffuse profile. The core exhibits a bright, yellow-orange hue, suggesting a population of older stars and/or dust obscuration. Surrounding the core, a fainter, greenish halo extends outwards, indicating the presence of a more dispersed stellar population or potentially ongoing star formation. No distinct spiral arms or bar structures are discernible. The overall morphology appears relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. The galaxy exhibits a generally elliptical shape, although some irregularity may be present in the outer regions.
