The galaxy presents as a late-type spiral, observed nearly edge-on. A prominent dust lane bisects the galactic disk, obscuring a significant portion of the starlight. The central bulge exhibits a soft, diffuse profile, appearing more rounded than boxy. It appears to be slightly skewed, with one side being slightly shorter than the other.

Based on the color indices, the bulge appears to exhibit a yellowish hue indicative of an older stellar population. Patches of blueish light are visible within the disk, likely regions of active star formation. The overall structure appears relatively undisturbed, with no obvious signs of recent major mergers, though minor tidal features cannot be entirely ruled out. The outer regions of the disk fade gradually, suggesting a relatively quiescent star formation history in those areas compared to the brighter, bluer patches. There is one notable region with a significant redder hue, most likely due to the presence of greater amounts of dust.
