The galaxy presents as a relatively smooth, elliptical-like structure. The galaxy's light is concentrated in the center, with a gradual falloff in intensity towards the edges. It exhibits a yellowish-red hue, suggesting an older stellar population and reduced ongoing star formation. There are hints of minor disturbances or asymmetries in the galaxy's shape, such as faint tidal tails or subtle irregularities in its outer regions; however, it is not currently undergoing a major merger. The galaxy is of intermediate size. 
