The galaxy appears as a relatively compact, smooth elliptical or lenticular structure. There is a high degree of central concentration of light, fading gradually towards the outer regions. Its overall color is yellowish. The observed smoothness suggests a generally older stellar population, though the color implies there is still some star formation present. No obvious spiral arm structures or significant dust lanes are visible in this image. There is no sign of any current mergers or major disturbances. Based on its morphology, this galaxy is likely a relatively evolved system with a substantial mass.
