The galaxy appears as a smooth, elliptical structure with a concentrated central bulge. The core exhibits a yellowish-orange hue, indicative of an older stellar population. Moving outwards from the core, the color transitions to a more diffuse, greenish-blue, which might suggest the presence of some younger stars or ongoing star formation, albeit at a low level. The galaxy displays a generally well-defined structure, with no obvious signs of major disturbances or mergers, though slight asymmetries might hint at minor gravitational interactions. It is moderately luminous, with a fairly compact size and no spiral arms.
