The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated with a gradual decrease in intensity outward from the core. The galaxy exhibits a slightly yellowish central region with an extended, more diffuse halo. There are no apparent spiral arm structures or prominent dust lanes visible within the galaxy's disk or halo, but some faint features might be very minor disturbances. The galaxy appears to be a relatively isolated object, with no obvious signs of recent major merger events. It has a medium mass and low star formation rate.
