The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The color gradient suggests an older stellar population, with the core exhibiting a yellowish hue. There is a noticeable lack of spiral arm structure. Some minor asymmetries or disturbances can be seen in the faint outer regions. These may be evidence of a past or ongoing minor interaction. Based on color and morphology, the galaxy seems to have low star formation activity. The overall shape is close to round.
