The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated light profile, with a gradual decrease in surface brightness moving outward from the core. The galaxy appears generally rounded, with a slight deviation from perfect circularity. There is little evidence of distinct spiral arm structures or significant dust lanes within the galaxy's disk. Faint blue hues are detectable within the galaxy, potentially indicating regions of recent, though somewhat limited, star formation. Overall, the galaxy appears relatively undisturbed, showing no prominent signs of ongoing or recent major merger activity. There is some weak evidence of a minor disturbance in the form of a tidal tail or plume. The overall mass appears small and has a low star formation rate.
