The galaxy presents as a spiral type, displaying a prominent disk structure. Two distinct spiral arms are clearly visible, exhibiting a tightly wound morphology around a central bulge. The bulge appears to be of moderate size compared to the overall galactic disk. The color distribution suggests a relatively low rate of on-going star formation activity within the disk and a redder bulge indicative of an older stellar population. There is no obvious evidence of recent merger activity or major disturbances in the galactic structure. The galaxy is observed nearly face-on, allowing for detailed observation of its spiral structure. A faint bar is suspected, but the evidence is too faint to confirm visually.
