The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that dominates the overall luminosity. The radial light profile decreases smoothly outward from the core. There is a subtle color gradient, transitioning from a yellowish-white core to a slightly bluer halo. No distinct spiral arms or bar structures are discernible. The surrounding halo appears relatively uniform, with a slight suggestion of extended structure, though not definitively indicative of any major ongoing merger activity. A minor disturbance may be occurring. The apparent roundness suggests a low inclination relative to the observer's line of sight. The object displays characteristics consistent with a quiescent galaxy, with a relatively low star formation rate.