The galaxy presents as a largely smooth, elliptical object with a luminous, concentrated central bulge exhibiting a yellow-white hue. A fainter, more diffuse structure is present in the immediate vicinity, suggesting a disturbed system or interaction of some kind. The primary galaxy has a high degree of roundness. There is potential evidence of minor disturbance in the disk, although no substantial tidal features or merging signatures are readily apparent. Overall, the galaxy appears relatively mature, with a low star formation rate. The galaxy's absolute magnitude indicates that it is relatively luminous.
