The galaxy presents as a smooth, elliptical morphology with a concentrated central bulge that emits a yellowish hue. This bulge appears to dominate the overall light output of the galaxy. Fainter, less concentrated light emanates from the outer regions, gradually diminishing in intensity with distance from the center. The galaxy exhibits a slight ellipticity, deviating marginally from a perfectly circular shape. No distinct spiral arms or prominent dust lanes are discernible. The overall impression is of an evolved stellar population with a relatively low rate of ongoing star formation, consistent with a passively evolving system at a redshift of approximately 0.34.
