The galaxy appears to be a spiral galaxy seen at an oblique angle. The disk component exhibits distinct color gradients, shifting from bluish hues on one side to reddish tints on the opposite. These color variations likely indicate differences in stellar populations and ongoing star formation activity, with the blue colors suggesting regions of recent or ongoing star formation and the redder colors suggesting older stellar populations. There is some evidence of a central bulge, slightly brighter than the surrounding disk. The bulge appears relatively smooth in texture, possibly indicating an older stellar population and a less active star formation history compared to the disk regions. Faint, disturbed morphology might suggest a possible interaction or minor merger event in its past. Overall, the galaxy presents a complex structure with evidence of varied stellar populations and a potentially dynamic evolutionary history.
