The galaxy exhibits an elliptical morphology, appearing largely smooth and featureless. It has a concentrated central bulge, which appears a yellow-orange hue, suggestive of an older stellar population. Moving outward from the core, the galaxy shows a diffuse, greenish halo with a faint disc, likely indicating a mix of stellar populations and some ongoing, though subdued, star formation. There is little evidence of prominent spiral arms or significant dust lanes. The overall appearance is consistent with a galaxy at intermediate redshift, showing no strong signs of recent major merger activity or significant tidal disturbances, though there may be some signs of minor disturbances.
