The galaxy presents as a luminous, elliptical morphology, with a concentrated central bulge that dominates its overall structure. The core is intensely bright, exhibiting a yellowish-white hue that suggests an older stellar population. The overall light distribution is smooth and relatively uniform, with the intensity gradually decreasing outwards from the center. A very slight flattening of the galaxy is observed, indicating a deviation from a perfectly spherical shape. The outer regions display a fainter, reddish tint. No distinct spiral arms, dust lanes, or other features indicative of active star formation are readily apparent. The galaxy appears relatively isolated and undisturbed.