This galaxy presents as an edge-on spiral. The disk appears relatively thin and elongated with a notable central bulge. The bulge exhibits a smooth profile, lacking any obvious substructure. A slight boxiness cannot be ruled out due to the resolution. No clear signs of active galactic nuclei or substantial dust lanes are apparent across the disk. The lack of merging characteristics implies a relatively undisturbed evolutionary history. The disk color exhibits a bluer tint than the bulge, suggestive of younger stellar populations within the disk compared to the older, redder stars populating the bulge. The galaxy’s overall structure suggests a high inclination angle relative to our line of sight. The smooth morphology suggests a mature system, potentially with a relatively high mass.
