The galaxy appears as a centrally concentrated system with a smooth, somewhat elliptical morphology. The core is a bright, yellow-white region, indicative of an older stellar population. Extending outward from the core, a fainter, more diffuse halo is observed. This halo exhibits a subtle colour gradient, with the inner regions showing a yellowish tint and the outer regions a slight bluer hue. No distinct spiral arms or other prominent features like dust lanes are discernible. There is no major ongoing merger apparent, but there may be minor tidal disturbances.
