This galaxy presents a clear spiral structure. Its morphology is disk-dominated, with a discernible, though relatively small, bulge at its center. The spiral arms appear well-defined, and the winding of these arms is of medium tightness. These arms appear to host a few regions of star formation. The orientation of the galaxy is nearly face-on relative to our line of sight. The disk exhibits a non-uniform color distribution, with subtle variations suggesting differences in stellar populations across the spiral arms. The bulge region appears to be a more uniform color, suggesting an older stellar population. There is no apparent evidence of a strong bar structure bisecting the galaxy. The overall appearance suggests a quiescent galaxy, with no major signs of ongoing merger activity or significant disturbances. The galaxy's visual properties suggest a mass intermediate between a dwarf and a giant galaxy.
