The galaxy presents as a moderately bright, disk-shaped system viewed at an oblique angle. It exhibits a central, slightly brighter bulge that appears relatively smooth. The disk component shows hints of spiral structure but lacks clear definition. The overall color appears bluish, suggesting the presence of a younger stellar population and ongoing star formation, with the possibility of a relatively low star formation rate. The galaxy exhibits a degree of disturbance in its morphology and may be undergoing a minor interaction or merger. The shape of the disk is not perfectly round, showing some asymmetry, although it does not appear highly elongated.
