The galaxy presents an elliptical morphology, appearing somewhat elongated with a smooth and featureless profile. Its core exhibits a high surface brightness concentration, suggesting a significant stellar density. The luminosity decreases gradually from the center outwards, with no discernible spiral arms or bar structures. There is a slight color gradient visible. The central region appears more yellow, potentially indicating an older stellar population, while the outer regions show a slightly bluer tinge. The image suggests that it is not currently undergoing any major merger events, and only exhibits a small hint of some kind of distortion or minor interaction.
