The galaxy presents as a spiral type, although the orientation is not perfectly face-on, and possibly a bit distorted, preventing clear observation of its structure. The central region appears elongated, suggesting the possible presence of a bar feature bisecting a small or indistinct bulge.

Spiral arms are present and appear relatively tightly wound. Patchy regions of star formation or dust are observed along the arms, appearing bluer in color. The disk component seems prominent and potentially disrupted, with signs of disturbances or tidal interactions. There is also a bright object near the center of the galaxy, likely either a concentrated region of the bulge or a background object. The overall color of the galaxy leans towards blue, which would be indicative of active star formation.
