The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms. The morphology suggests a substantial disk component oriented nearly face-on. The galactic bulge is clearly visible, exhibiting a moderate size relative to the overall galactic structure. A bar structure appears present within the central region. The spiral arms appear to exhibit a medium degree of winding. The arm structure appears to be dominated by two spiral arms. Visual inspection does not reveal any signs of major mergers. However, some disturbances exist that suggest minor gravitational interactions with another galaxy are possible. The colour profile suggests the presence of active star formation, particularly within the spiral arms.
