The galaxy appears to be an elliptical or lenticular type, displaying a smooth, concentrated central bulge with a gradual decrease in luminosity towards the edges. The galaxy exhibits an elongated shape, with an axis ratio suggesting it is viewed at an oblique angle. The light distribution is predominantly smooth, indicative of an older stellar population. A subtle disk-like structure may be present but is not clearly resolved. No prominent spiral arms or dust lanes are visible. There is a hint of bluer star formation at the outer edges of the galaxy. No strong tidal features or signs of recent major mergers are apparent.
