The galaxy presents as a flattened, elliptical morphology, viewed at an oblique angle relative to its major axis. The central region exhibits a smooth, concentrated luminosity profile, appearing yellowish-orange in color, likely indicating an older stellar population. Moving outwards from the core, the galactic disk exhibits a gradual decrease in luminosity with more diffuse and cooler colors, transitioning to greener hues, which may indicate the presence of younger stars and active star forming regions. The galaxy does not show any major disruptions, tidal tails, or other evidence of a recent major merger event; it appears to be relatively undisturbed. The overall structure suggests an elliptical or lenticular galaxy type, with ongoing, moderate star formation activity in the outer regions.
