The galaxy presents a somewhat irregular morphology. There is a dominant, brighter region, likely the galactic nucleus or a region of concentrated star formation. This region exhibits a bluer hue, suggestive of a younger stellar population with hotter, more massive stars, therefore possibly active star formation. The light distribution extends outwards from this brighter region with hints of fainter features and lower surface brightness components. These seem to be in the early stages of interacting or merging with another galaxy. There are minor disturbance visible, but the system seems to be relatively well conserved. There is a slight redshift, indicating that it is further than our own galaxy. The galaxy is mostly smooth, not showing any signs of spiral arms.
