The galaxy presents as a disk galaxy, potentially with spiral structure, though the arms are not sharply defined. There is a central bulge region, but it doesn't appear overly prominent. The galaxy has a generally smooth appearance with some features of an actively star forming galaxy. There is a very slight likelihood of this galaxy merging. The blue hue suggests ongoing star formation within the galaxy. The relatively high concentrations of blue stars, coupled with the estimated size, suggest a relatively young or actively star-forming galaxy. The light is most intense in the galactic center.
