The galaxy appears as a smooth, centrally concentrated object with an elliptical morphology. The light distribution suggests a bulge-dominated system. The core exhibits a yellowish hue, potentially indicating an older stellar population. The overall shape seems relatively regular, showing no signs of major tidal disturbances or ongoing mergers, although a slight asymmetry might suggest minor gravitational interactions. The disk is inclined relative to our line of sight. There is a faint disk surrounding the bulge that is somewhat more blue in color, suggesting younger star populations.
