The galaxy presents as an edge-on spiral system. A central bulge is apparent, exhibiting a somewhat elongated and mildly boxy morphology. The galactic disk appears thin and extended, bisected by a prominent dust lane. The color profile suggests active star formation within the disk, indicated by the bluer hues. Overall, the galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or significant tidal interactions. Star formation is seemingly low. The stellar mass is estimated to be quite high.
