The galaxy presents as an edge-on spiral, or possibly a lenticular galaxy, viewed from Earth. A distinct central bulge, exhibiting a yellowish hue indicative of an older stellar population, dominates the galaxy's core. From the central bulge, a flattened disk extends outward, appearing bluish in color. This blue tint implies the presence of younger, hotter stars and ongoing star formation within the disk. The galaxy's disk appears largely undisturbed, showing no obvious signs of interaction or recent major merger events. The lack of prominent dust lanes and the relatively smooth appearance suggests a galaxy that has undergone a period of relative quiescence in terms of major starburst activity. The galaxy exhibits a fairly regular morphology without any obvious asymmetry or tidal features. Its overall structure suggests a gravitationally stable and relatively evolved system.
