The galaxy presents as a moderately luminous, relatively compact object. Its morphology appears largely smooth and elliptical in nature, with a high degree of central concentration. There is a suggestion of a slight color gradient, shifting from a generally redder core to a bluer halo. Subtle irregularities exist within the smooth structure, possibly indicating minor disturbances. A very slight asymmetry may be present, hinting at a potential past or ongoing minor interaction. The galaxy lacks prominent spiral arms or a distinct disk. The overall form points towards an evolved system, consistent with a galaxy where star formation has slowed.
