The galaxy presents a generally smooth, elliptical morphology. The dominant feature is a bright, concentrated central bulge exhibiting a yellowish-orange hue, indicative of an older stellar population. Fainter, bluer regions suggest the presence of some younger stars toward the outer edges of the disk. The overall structure appears relatively undisturbed with no signs of major merging events or tidal tails. The galaxy is approximately 8 kpc in radius. It is a high mass galaxy.
