The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The galaxy appears more rounded than elongated, with no prominent spiral arm structures or dust lanes visible. There is evidence of a possible minor disturbance or interaction, as suggested by a slight asymmetry in the isophotes. Color indices indicate that the galaxy is dominated by an older stellar population, exhibiting a reddish hue. The overall light distribution is consistent with that of an early-type galaxy with low ongoing star formation.
