The galaxy presents as a relatively smooth, elongated structure with a cigar-like shape. It displays a central bulge that is not particularly prominent, with a disk that appears to be viewed at a high inclination, near edge-on. The galaxy exhibits a pale blue hue along its main body, suggesting the presence of younger, hotter stars and ongoing star formation. There's a slight suggestion of patchy light distribution within the disk, indicating possible spiral arm structures, but resolution limitations prevent a definite identification. No obvious signs of major disturbances or mergers are visible, although minor asymmetries may exist. Overall, this galaxy appears to be a relatively undisturbed, disk-dominated system with a moderate degree of ongoing star formation.
