The galaxy appears to be a spiral galaxy seen edge-on. It presents a somewhat smooth, elongated profile. There is a noticeable bulge that dominates the central region, exhibiting a bright, concentrated luminosity. The disk is visible as a fainter, bluish haze extending outwards from the bulge. The edges of the disk are not sharply defined, suggesting a gradual decrease in stellar density with increasing distance from the center. There is no clear evidence of strong spiral arm structure, likely due to the edge-on viewing angle. No significant signs of tidal disturbances or ongoing merger activity are apparent.
