The observed galaxy presents an elliptical morphology with a bright, concentrated central bulge. The light distribution appears smooth and centrally concentrated. The galaxy exhibits a blue-ish halo and a bright white core, suggestive of active star formation or an active galactic nucleus. There is little evidence of distinct spiral arms or a well-defined disk. The observed light distribution suggests a relatively uniform stellar population throughout the galaxy. There appears to be a tidal feature or minor disturbance that causes asymmetry on the periphery of the halo of the galaxy.
