The galaxy appears to be a spiral galaxy, seen at an oblique angle. The central bulge is a pronounced yellowish-orange color, suggesting an older stellar population. The disk shows hints of spiral arm structure, with regions of bluer emission indicating areas of active star formation. The disk has a general distribution of color from light blue to green to dark red as you move away from the core. Overall, it seems the galaxy is relatively smooth in appearance, with no major signs of disruption or tidal interactions. The galaxy exhibits an elongated shape, with a roughly estimated physical radius around 5 kpc.
