The observed galaxy presents a complex morphology. It appears to be a spiral galaxy, exhibiting subtle spiral arm structures, though they are not sharply defined. The galaxy possesses a notable central bulge, moderate in size, appearing luminous and concentrated. The overall disk appears tilted slightly relative to the observer's line of sight. No bar structure is readily apparent. No major signs of mergers or significant disturbances are visible. Overall, the galaxy seems to be relatively undisturbed in its current state.
