The galaxy presents as a relatively compact object with a dominant central bulge. The overall morphology appears to be somewhere between a disk galaxy and a smooth elliptical galaxy. The light distribution is concentrated toward the center, with a gradual decrease in intensity outwards, although there are small disturbances to the structure. The galaxy exhibits a slightly elongated shape. There appears to be a faint, disk-like structure surrounding the bulge, possibly with some spiral arms or other features, however these are quite faint. There is a slight color gradient observed across the galaxy, with a bluer hue toward one side, and redder hues on the opposite side, indicating areas of potential star formation and older stellar populations, respectively. It is likely undergoing some form of minor disturbance or interaction.
