The galaxy presents as a spiral, exhibiting a disk structure with prominent spiral arms. These arms are traced by regions of bluer light, indicative of ongoing star formation. The central bulge appears moderately sized and yellowish in color, suggesting an older stellar population. The spiral arms display a winding pattern classified between medium and loose. Two distinct arms are clearly visible. There is some suggestion of a bar-like structure running through the bulge. The galaxy shows slight signs of tidal disturbance or interaction, as evidenced by some asymmetry in the outer regions of the disk. The morphology of the spiral arms implies it is not an early stage spiral galaxy.
