The object presents as a spiral galaxy. It exhibits a central bulge region with a relatively compact and bright core, surrounded by a fainter, more diffuse disk. The spiral arms are well-defined and show a multi-armed structure. Traces of blueish hues, possibly representing regions of active star formation, are evident within the arms. The galaxy appears face-on with a slight inclination, allowing for good visualization of the spiral structure. The galaxy does not seem to be undergoing any major merging events, though some irregularities in the arm structure might indicate minor gravitational interactions. A weak bar structure seems to be present in the galaxy. The spiral arms appear moderately wound. The extent of the galaxy suggests it is an intermediate-sized spiral.
