This galaxy presents as a roughly elliptical, though not perfectly spherical, object. It exhibits a bright central core, possibly indicating the presence of an active galactic nucleus or a dense concentration of stars. The galaxy's color profile seems to lean toward the blue end of the spectrum, which could be indicative of ongoing star formation activity within the galaxy. However, there is also evidence of older stellar populations, given the central brightness, suggesting a mix of stellar ages. The morphology appears relatively undisturbed, though there are subtle irregularities in the outer regions of the galaxy. These irregularities hint at a possible past interaction or merger event. There are no clear spiral arms visible, the galaxy seems to be relatively small in size.
