The galaxy presents as a disk-shaped structure viewed at a moderate inclination. The central region exhibits a high degree of luminosity, appearing nearly spheroidal and transitioning gradually into a more diffuse and extended disk. The color profile shows a concentration of redder hues towards the center, suggesting an older stellar population in the galactic bulge. The outer regions of the disk are bluer, likely indicating ongoing or recent star formation.

There is subtle evidence of spiral arm structure, although it's not sharply defined. A slight asymmetry in the disk is observed, hinting at a possible past interaction, although no strong tidal features are immediately apparent. The galaxy appears relatively undisturbed, displaying a generally smooth and regular morphology.
