The galaxy presents as a spiral type with a disk that is close to face-on relative to our line of sight. Spiral arm structures are visible, though somewhat diffuse and not sharply defined. The arms appear somewhat flocculent. A central bulge is present, exhibiting a moderate size relative to the overall disk. There is no evidence of a strong bar structure bisecting the bulge. The galaxy's overall color profile suggests ongoing star formation. There is no obvious indication of a major merger event, though some minor disturbances or tidal features cannot be ruled out based on the image. The galaxy appears to be neither perfectly smooth nor completely dominated by disk features, implying a moderate degree of structural complexity.
