The galaxy presents as a spiral type, with a moderately sized bulge relative to the disk. The spiral arms are prominent, exhibiting a winding structure that transitions from tightly wound to medium. Two dominant arms are observed. There is also evidence suggesting the presence of a bar structure in the central region. The galaxy appears to have been undisturbed by major merging events, presenting a coherent structure. The galaxy is not edge on, but rather at an angle. The galaxy presents a modest rate of star formation.
