The galaxy exhibits a roughly elliptical morphology, with a bright central nucleus. There appears to be some sort of disk-like structure around the central region. The color gradient suggests the presence of different stellar populations, with bluer colors concentrated toward the center and a shift toward redder hues in the outer regions. The observed color distribution hints at ongoing or recent star formation activity, possibly concentrated in the central regions. There is a slight suggestion of asymmetry, indicating a minor disturbance or interaction with a nearby galaxy. 
