The galaxy presents a morphology consistent with a spiral galaxy. It exhibits a noticeable central bulge that appears moderately sized. Distinct spiral arm structures are evident, displaying a winding pattern that transitions from tightly wound in certain areas to more open in others. The galaxy's disk appears to be viewed at a slight inclination. There is a suggestion of a bar structure traversing the central region. No significant signs of ongoing major mergers or strong tidal disturbances are immediately apparent, though minor disturbances cannot be ruled out. Overall, the galaxy appears to be a relatively isolated spiral galaxy.
