The galaxy appears as a disk galaxy, viewed edge-on. A central bulge is evident, with a concentrated and bright core region that fades in intensity radially. The bulge exhibits a yellowish-orange color, indicating an older stellar population, with less recent star formation. A flattened disk structure extends outward from the central bulge. This disk component displays a bluer hue, suggesting the presence of younger, hotter stars and ongoing star formation, especially at the far ends of the disk. Overall, the galaxy possesses an elongated, cigar-like appearance, with a seemingly smooth overall structure, and no obvious signs of major mergers or strong tidal disturbances. The galaxy has low level star formation throughout the disk, but little to none in the center bulge. 
