The galaxy presents as a somewhat elliptical, though moderately rounded, structure. It appears to exhibit a significant central bulge that is yellow-white in color. This bright core is suggestive of a high concentration of older stars. Fainter, bluer light surrounds the core, hinting at younger stellar populations and potential ongoing star formation. Some irregular light distribution can be seen throughout the galaxy. Overall, this galaxy's morphology is suggestive of a galaxy undergoing or having undergone some kind of disruptive event.
