The galaxy appears to be a spiral galaxy, exhibiting a disk-like structure with a moderate bulge. Its orientation is nearly edge-on, allowing for a clear view of the flattened galactic disk. Prominent spiral arms emanate from the central bulge and extend outwards, displaying a tightly wound morphology. The galaxy possesses a slightly asymmetrical shape and a significant amount of internal dust. The spiral arms show a patchy distribution of star formation, with regions of enhanced brightness, likely indicating the presence of HII regions and ongoing star formation activity. A faint, extended halo may surround the galaxy, though this is difficult to ascertain with complete certainty.
