The galaxy presents as an edge-on disk galaxy with a notable dust lane obscuring the central bulge. The bulge appears relatively prominent and has a yellowish hue, potentially indicating an older stellar population. The disk exhibits a bluer color, suggesting the presence of ongoing star formation. The galaxy appears to be relatively smooth with some indication of disturbances in the disk. Based on the edge-on orientation, a significant fraction of the galaxy likely consists of disk components. There is no major merging activity occuring, but the asymmetry of the disk suggests some gravitational interaction.
