The galaxy presents an overall spheroid morphology with a dominant central bulge. The light from the galaxy has a distinctly bluish hue in the center, possibly indicating the presence of ongoing star formation or a population of young, hot stars. The outer regions of the galaxy appear more yellowish, which could be due to an older stellar population. There is little visual evidence of a pronounced disk structure, and no spiral arms are readily apparent in the image. No obvious signs of strong tidal interactions or major mergers are seen in the image.
