The galaxy presents as a moderately inclined, disk-like structure with a somewhat diffuse morphology. A central bulge region appears present, exhibiting a higher surface brightness than the surrounding disk. There are hints of spiral arm structures, but they are not sharply defined and appear flocculent. Blue hues are visible, concentrated primarily within the disk, suggesting ongoing star formation. The overall structure is somewhat irregular, possibly indicating tidal interactions or recent minor mergers. There appears to be a tail on the bottom left side of the galaxy, which is possibly caused by gravitational interaction. The galaxy is relatively isolated in the image, without any immediately apparent companion galaxies.
