The galaxy appears to have a relatively small angular size on the sky. The light profile indicates it is not entirely smooth, and instead shows some features. These features suggest there is a disk component. The primary body of the galaxy exhibits a bright, central concentration, which is typical of galaxies. The distribution of light within the galaxy shows variations in color, with a prominent green-blue tint dominant. This tint may indicate regions of active star formation. The shape is somewhat irregular, suggesting it may be an interacting galaxy, or experiencing some kind of minor disturbance. The morphology might represent a minor merging event. The merging object may be to the south of the galaxy. 
