The galaxy presents as a largely smooth object with a radial profile that brightens significantly toward the center. The core is luminous, and the overall shape appears round. The image does not obviously show any spiral arm structure, strong tidal features, or signs of a major merger. There are minor signs of disturbances in the outer regions of the galaxy. Based on these features, it is likely the galaxy has a significant spheroidal component. There appears to be ongoing, but low, star formation within the galaxy. The galaxy has an estimated stellar mass of approximately 10^10 solar masses.