The galaxy presents an elliptical morphology with a centrally concentrated bulge. The core exhibits a high degree of luminosity, with a gradual decrease in brightness moving outward towards the edges of the galaxy. It displays a flattened shape with a major axis oriented approximately vertically in the image. The galaxy exhibits a relatively smooth appearance with no distinct spiral arm structures. The overall color suggests a stellar population that is likely composed of older, redder stars in the bulge, with the outer regions possibly indicating the presence of younger, bluer stars. There is a hint of some dust obscuration in the outer regions of the galaxy. There is no evidence of an active galactic nucleus. Overall, the galaxy appears as a relatively undisturbed, evolved system.
