The galaxy appears to have a dominant, smooth central bulge. The light from the central region is concentrated and exhibits a yellowish hue. Adjacent to the central bulge is a secondary, less prominent structure that displays a bluer color. This bluer region may indicate areas of active star formation. There is evidence of faint tidal distortions, potentially suggesting an ongoing or recent interaction with another galaxy. The overall shape of the galaxy is somewhat elliptical, with the light distribution becoming more diffuse at the outer edges. The light is distributed relatively evenly, with no spiral arms clearly visible.
