The galaxy appears to be a spiral galaxy seen at a moderate inclination angle. The central bulge is prominent and exhibits a yellow-orange hue, possibly indicating an older stellar population. The disk is visible and shows some evidence of spiral arm structure, although the arms are not sharply defined. The galaxy is relatively smooth in appearance, with no obvious signs of major mergers or tidal disturbances. The galaxy's light is concentrated towards the center, with a gradual decrease in brightness towards the outer regions. The color gradients suggest ongoing star formation in the disk, but at a relatively low rate. Overall, the galaxy appears to be a relatively normal spiral galaxy undergoing quiescent evolution.
