The galaxy appears as a somewhat elliptical, concentrated light source. It exhibits a smooth, featureless structure with no readily discernible spiral arms or distinct morphological characteristics typically associated with late-type galaxies. The central region is more luminous, suggesting a higher stellar density or active galactic nucleus activity. There may be a faint tidal tail or stream emanating from the galaxy to the left, which could indicate a past or ongoing interaction with another galaxy. The overall color is dominated by yellow-green wavelengths, possibly indicating an older stellar population with lower levels of recent star formation.
