The galaxy presents as a generally smooth, elliptical-like object with a concentrated central bulge. There are no distinct spiral arm structures visible. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a bluer periphery. This suggests older stellar populations are centrally located, with younger, bluer stars more prevalent in the outer regions. A slight elongation is perceptible along its major axis. There appears to be some level of gravitational disturbance in the lower right quadrant.
