The galaxy presents as a slightly inclined spiral, displaying a prominent central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. Fainter, bluish spiral arms extend outwards from the bulge, indicative of ongoing, but relatively low, star formation. The disk of the galaxy appears relatively smooth. There are no obvious signs of any major recent merger events, although there seems to be some disturbance within the arms. Dust lanes are not easily discernible, but some mottled areas and color variations within the arms could indicate their presence.
