The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a concentrated luminosity profile, suggestive of a significant stellar bulge. The color gradient indicates a shift towards bluer hues in the outer regions compared to the more red-dominated central bulge, implying ongoing star formation within the galactic disk. The surface appears mostly smooth, with a subtle hint of a disk-like structure. No prominent spiral arms or bars are discernible. There is no indication of a significant ongoing merger or tidal disturbances.
