The galaxy presents as a spiral with a prominent central bulge, appearing yellowish, suggesting an older stellar population in this region. The spiral arms are loosely wound and somewhat patchy in appearance, with varying concentrations of bluer light, indicating ongoing star formation. One arm appears more disrupted compared to the other, hinting at a possible interaction or past merger event. The galaxy's overall shape is somewhat elongated. There is a nearby dwarf galaxy that seems gravitationally bound to the larger galaxy. 