The galaxy presents as an edge-on spiral, with a distinct disk structure bisecting a central bulge. The disk appears relatively thin and exhibits subtle color variations, suggesting the presence of spiral arms obscured by the viewing angle. These arms are likely undergoing active star formation, indicated by the slight bluer hue in sections of the disk. The central bulge displays a smoother, more uniform orange color, indicative of an older stellar population. There is no clear indication of a strong active galactic nucleus, though the bulge appears moderately luminous. Overall, the galaxy appears to be a fairly massive disk galaxy that is actively forming stars at a modest rate. The morphology suggests no recent major merger events, though minor disturbances cannot be completely ruled out. The bulge profile is mostly rounded.
