The galaxy presents a generally smooth, elliptical morphology, exhibiting a concentrated central bulge that transitions into a less dense outer halo. The color appears somewhat blue, potentially indicating the presence of relatively young stars and ongoing star formation. However, the galaxy is mostly smooth and features a round shape with no defined spiral arm structures or significant dust lanes visible. There are no prominent tidal tails or distorted features suggesting recent major merger events. The overall appearance suggests a system undergoing only minor disturbances, but potentially some merging activity based on a slight asymmetry of the halo.
