This galaxy exhibits a generally smooth morphology, with a slight elongation. The galaxy is predominantly a central bulge with what appears to be a disk component with spiral arms. A bright, concentrated nucleus is present. The color is a mix of blue and white, suggesting a population of young, hot stars along with older stars. There is an indication of a possible interaction or merging event as there is a small amount of light present to the top left. This indicates this galaxy is in the process of merging with another galaxy, or maybe a smaller dwarf galaxy. Overall, this galaxy presents as an intermediate mass system with some ongoing star formation, and possible interaction with another galaxy.
