The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a notable central bulge with a concentrated, bright core, which appears yellowish, suggesting an older stellar population. The overall shape is somewhere in between round and elliptical. The disk component, if present, is not well-defined; there is faint indication of a disk plane. The galaxy does not show any obvious signs of major disturbances or ongoing merging activity. No distinct spiral arms are visible, and the light distribution appears largely uniform aside from the central concentration.
