The galaxy presents as a spiral structure with a notable central bulge, but exhibiting significant disturbances. The arms are not well-defined, appearing flocculent rather than grand design. There is evidence of asymmetry within the disk, possibly indicative of gravitational interactions or recent merger events. A portion of the galaxy appears diffuse and irregular, suggesting ongoing star formation. The color distribution reveals a dominant blue hue, particularly in the outer regions, likely due to the presence of younger, hotter stars. The disk of the galaxy is slightly tilted with respect to the line of sight.
