The galaxy presents as a slightly elongated, lenticular or elliptical structure. The core exhibits a concentrated, bright yellow-orange hue, indicating an older stellar population likely dominating the central region. Moving outwards from the core, the galaxy displays a gradual decrease in luminosity. Some faint and diffuse blue light can be observed especially at the furthest points from the core. The overall morphology appears largely undisturbed, with no obvious signs of major mergers or significant tidal interactions. The galaxy appears smooth and somewhat round.
