The galaxy appears as a centrally concentrated, elliptical or lenticular system. It is characterized by a smooth, mostly featureless morphology. The light profile transitions smoothly from a bright, yellowish core outwards, with a gradual decrease in intensity. The isophotes appear mostly round with a small amount of distortion. There are some indications of bluer hues in the outer regions of the galaxy, hinting at pockets of star formation. The galaxy lacks any strong spiral arm structures or distinct dust lanes. There is no evidence of a recent major merger event, however, there is a slight distortion which could indicate minor disturbance from a past merger event. The galaxy's color suggests it is a relatively evolved system with an intermediate to low star formation rate. Overall, it appears to be a quiescent galaxy of intermediate mass.
