The galaxy presents a primarily smooth morphology with a central bulge that appears more luminous than the surrounding disk. The overall shape is elliptical, deviating slightly from a perfect circle towards a more elongated, cigar-like appearance. There is subtle evidence of a faint, extended disk surrounding the central bulge. Within the disk, the light distribution appears relatively uniform, without prominent spiral arm structures. The color gradients suggest that the core is older and redder in comparison to the disk. The galaxy lacks any prominent features indicative of major mergers. Minor disturbances or interactions cannot be completely ruled out due to some irregularities observed in the outer regions. The morphology is dominated by a smooth central component which indicates an elliptical-like nature.