The galaxy presents as a diffuse, centrally concentrated object. Its overall color is bluish, with an apparent smooth morphology, lacking distinct spiral arms or a prominent bar structure. There is evidence of a possible minor disturbance, with some asymmetry observed in the outer regions of the galactic disk, suggesting a possible past or ongoing interaction. The galaxy is relatively compact, exhibiting a high degree of roundness. Its light profile appears somewhat uniform, hinting at a relatively homogeneous stellar population. The galaxy shows evidence of ongoing, but relatively low, star formation. Overall, it appears to be an elliptical or early-type spiral galaxy at a moderate redshift.
