The galaxy presents as a cigar-shaped or highly elongated structure. It exhibits a smooth, diffuse light distribution across the main body. A central bulge is faintly visible, showing a subtle concentration of light. The color gradient transitions from a yellowish-white core to a bluer hue at the edges, suggesting a possible mix of older stellar populations in the center and younger, bluer stars in the outer regions. No distinct spiral arm structures are discernible. There is no evidence of major mergers or significant tidal disturbances. It appears to be a relatively isolated system.
