The galaxy presents as a moderately bright, elliptical-shaped object, appearing largely smooth in structure. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. A subtle color gradient is observed, transitioning from a warmer, possibly older stellar population in the core to slightly cooler, possibly younger stellar populations in the outer regions. There is a hint of a disk-like structure, although features appear subdued. Faint irregularities are present, indicating a slight disturbance in the galaxy's morphology, possibly from minor interactions. Based on morphology, the galaxy doesn't seem to be undergoing major mergers.
