The galaxy presents as an elongated, edge-on spiral galaxy with a notable dust lane bisecting its major axis. The central bulge is prominent and appears to have a rounded morphology. Light distribution suggests that the galaxy disk is the dominant feature. There is some asymmetry visible which could indicate minor disturbances or interactions with a companion galaxy, or it may be internal structure. The blue hue in the outer regions could indicate ongoing star formation. Overall, the galaxy seems to be a relatively typical example of a spiral galaxy seen from an edge-on perspective, possibly showing some evidence of activity.
