The galaxy presents as a disk-shaped system, viewed at a moderate inclination relative to our line of sight. A central bulge is discernible, appearing brighter and more condensed than the surrounding disk. The disk exhibits a degree of asymmetry, with variations in surface brightness along its extent. A slight disturbance may be present. The overall color is bluish, suggesting the presence of a population of young, hot stars within the disk. There is no clear spiral structure visible at this resolution, but the disk appears somewhat flocculent. The galaxy appears relatively isolated, showing no signs of significant interaction with other galaxies.
