The galaxy exhibits a centrally concentrated morphology. The core appears bright and relatively smooth, transitioning into a more diffuse halo. The overall form is generally elliptical, appearing close to circular, with a slight deviation towards a prolate shape. There is some visual evidence of a minor interaction or disturbance influencing the galaxy's structure, with possible tidal features or asymmetries present. A secondary component, indicated by a region of orange light, is adjacent to the main body of the galaxy, potentially representing a region of enhanced star formation or another galaxy in the process of merging. Overall the galaxy is a relatively high mass object with a moderate degree of recent star formation.
