The galaxy presents a somewhat elongated morphology, appearing nearly edge-on from our vantage point. A bulge is visible at the center of the galaxy, exhibiting a smooth, centrally concentrated luminosity profile. The galaxy shows a disk. Based on its color profile, the central bulge appears to be populated by older stellar populations. Fainter arms extend outwards into a disk. There are no significant signs of ongoing merging activity or major disturbances in the galaxy's overall structure. 
