The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated luminosity profile. There is a lack of discernible spiral arm structure. The primary color of the galaxy is yellowish-orange. The is some evidence of a potential tidal tail or distortion extending outward from the main galactic body. The core of the galaxy appears particularly bright, suggesting a concentration of older stars. Star formation rate appears low based on its color. The overall shape is largely round. Some evidence of disturbance is seen, but it is not particularly strong. 
