The galaxy presents an elliptical morphology, elongated along its major axis. The central bulge exhibits a bright, concentrated luminosity profile, appearing smooth and yellowish. A fainter, less defined disk-like structure surrounds the bulge, displaying a subtle gradient in surface brightness from the inner to outer regions. Faint hints of bluer tones are detectable within the disk, possibly indicating regions of recent or ongoing star formation, although these are not prominent. The galaxy appears relatively undisturbed with no clear signs of major mergers or tidal features. Its overall structure suggests a mature system, likely dominated by an older stellar population, with potential for some residual star formation within the disk component.
