The galaxy presents as a relatively smooth, elliptical structure, viewed nearly face-on. The central region exhibits a high surface brightness, with a concentrated, possibly actively galactic nucleus appearing yellow-white in color. Surrounding the core, a more diffuse halo extends outwards, displaying a subtle color gradient that transitions from yellow-green in the inner regions to a bluer hue in the outer regions. This suggests a distribution of stellar populations, with older, redder stars concentrated in the central bulge, and younger, bluer stars populating the outer halo. There is no discernible dust lane or spiral arm structure visible, supporting its classification as an elliptical galaxy. The galaxy appears to be relatively isolated, showing no obvious signs of tidal interactions or major disturbances. Its overall morphology indicates a system likely undergoing relatively quiescent evolution.
