The galaxy appears to be an edge-on disk galaxy, presenting a clear, flattened structure. A prominent central bulge is visible, displaying a bright, concentrated luminosity. This bulge transitions into a disk, exhibiting a reddish hue suggestive of older stellar populations. 

The disk shows evidence of dust lanes, particularly along the central plane, contributing to its complex structure. There may be some tidal disturbances or distortions suggestive of a minor merger or interaction.

A faint, extended halo or outer disk component is tentatively discernible, encompassing the main body of the galaxy, though its precise morphology is difficult to ascertain. The overall color gradient suggests active star formation is occurring, but is likely in a declining stage.
