The galaxy presents as a somewhat elongated, possibly disk-like structure viewed at an oblique angle. The central bulge appears relatively prominent and concentrated, exhibiting a yellowish-orange hue. Extending from the central region are fainter, less defined arms or extensions, hinting at a spiral or barred-spiral morphology, though the resolution limits definitive classification. There appears to be some disturbances in the arms of the galaxy, with some asymmetry and irregularities present. The galaxy appears reddish than other parts of the image, indicating either an older stellar population, dust obscuration, or a higher redshift. Overall, the galaxy appears to be relatively isolated, with no immediately obvious signs of major interaction, although minor tidal features or satellite galaxies cannot be ruled out given the image quality.
