The galaxy presents as a lenticular or edge-on spiral, with a notable central bulge. The primary disk component is oriented near edge-on, making it difficult to discern detailed spiral arm structure. The bulge appears concentrated and exhibits a yellowish-white hue, potentially indicating an older stellar population or a significant dust component. A fainter, bluish halo extends along the major axis. The edge-on orientation allows for investigation of dust lane presence and bulge morphology. There is no obvious evidence of a major merger or significant tidal disturbance, though slight irregularities in the disk profile may suggest minor interactions. The color gradients within the galaxy suggest differential stellar populations and dust distribution. The overall morphology points toward a system that may be actively star-forming.
