The galaxy presents a generally smooth appearance, with a slightly elongated, cigar-shaped morphology. The central bulge exhibits a yellowish hue, indicating a higher concentration of older stellar populations. Moving outwards from the center, the galaxy gradually transitions to a bluer color, suggesting the presence of younger, hotter stars within the disk. There is little to no apparent spiral arm structure visible in the image. There are no obvious signs of tidal disturbances or major mergers. The galaxy is likely a relatively quiescent system with moderate star formation activity.