The galaxy presents as a spiral galaxy, though with an irregular morphology suggesting possible gravitational interactions. The disk appears inclined relative to our line of sight but is not edge on. The galactic bulge is not prominent, appearing small or non-existent. Spiral arms are visible but not well-defined. The arms have a patchy structure with localized regions of intense star formation. These regions are notably bluer in color, potentially indicating a younger stellar population. There is evidence of disturbances that are likely caused by a merging event. The central region of the galaxy is obscured by dust. There is no clear bar feature.