The galaxy presents a smooth, elongated morphology, appearing cigar-shaped. There is a notable absence of well-defined spiral arm structures or intricate details within the disk, suggesting it may be either an elliptical galaxy or a lenticular galaxy viewed edge-on. The primary body of the galaxy exhibits a color gradient, with the central region displaying a slightly yellower hue compared to the bluish outer edges. This suggests a higher concentration of older stellar populations in the galactic nucleus and the presence of younger, bluer stars in the peripheral regions. There is no obvious evidence of major ongoing mergers or tidal disturbances. The overall structure is relatively undisturbed, with only subtle asymmetries that might indicate minor interactions or internal processes.
