The galaxy presents a generally smooth appearance, but appears more elongated than circular, with hints of internal structure. The color gradient suggests a possible presence of an aging stellar population and a lower rate of star formation in the central regions. The galaxy appears to have a moderate inclination angle relative to our line of sight. The overall light distribution suggests a centrally concentrated mass profile, and it is likely an elliptical or lenticular type galaxy. There is a slight color variation visible within the galaxy, with a possible subtle bluer tinge toward the outer regions of the galaxy.
