The galaxy presents as an edge-on spiral, exhibiting a prominent dust lane bisecting the elongated galactic disk. A central bulge dominates the visual morphology, appearing smooth and somewhat rounded. The disk component shows hints of structure, but lacks distinct spiral arm definition in the available imaging. There is no morphological evidence suggesting any recent or ongoing major merger activity. The galaxy appears relatively isolated. The color profile suggests that the bulge exhibits a relatively older stellar population, while the disk may contain pockets of more recent star formation activity.

