The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a smooth, diffuse appearance with a distinct yellowish-orange hue, suggestive of an older stellar population. Fainter, bluish tones are observed at the periphery, potentially indicating regions of more recent star formation, however the blue light appears faint. No distinct spiral arm structures or prominent dust lanes are discernible at this resolution. Overall, the galaxy appears relatively undisturbed, with no immediately obvious signs of major mergers or interactions. The galaxy's light distribution is dominated by the central bulge.
