The galaxy presents as a smooth, elongated structure, appearing cigar-shaped in morphology. There is a central, bright core that fades gradually outward, suggesting a relatively high concentration of stars or other luminous material towards the center. No distinct spiral arms or prominent dust lanes are visible. The overall color appears somewhat homogenous, with a slight bluer tint to the nucleus. There is no visual evidence of any major interactions or mergers with other galaxies, although there is a subtle asymmetry that may indicate minor disturbances.
