The galaxy appears to be a spiral galaxy, viewed nearly edge-on from our perspective. It exhibits a flattened disk shape with a prominent central bulge. The bulge shows a smooth, concentrated luminosity profile, with a yellowish hue, likely indicating an older stellar population. The disk is relatively thin, with the majority of the light concentrated in a narrow plane. The disk shows slight color variation, appearing bluer towards the edges, suggestive of ongoing star formation activity. Dust lanes are not clearly visible, but there might be subtle obscuration within the disk. There is no obvious evidence of any major merging activity.
