The galaxy presents as a centrally concentrated system with a smooth overall morphology. There is a bright, yellowish core, which likely indicates an older stellar population dominating the central region. The light from the core fades gradually outwards, transitioning into a fainter, more diffuse halo. The halo exhibits a subtle bluish tint, hinting at the presence of some younger, hotter stars or ongoing star formation. Overall, the galaxy appears relatively undisturbed, with no obvious signs of tidal features or major interactions. There may be minor disturbances however, as there are slight asymmetries visible within the diffuse halo.
