The observed galaxy appears to be a spiral galaxy, likely at an intermediate redshift. It presents with a defined central bulge, exhibiting a yellow-orange hue, suggestive of an older stellar population. The disk component is visible but somewhat diffuse, with a bluish tint suggesting more active star formation. Two spiral arms are distinctly observed, appearing somewhat loosely wound. There may be faint indications of a bar structure within the central region, however the resolution limits a definitive identification. The overall morphology indicates it is not undergoing any major merging events, although there is a possibility of minor disturbances in the disk. The galaxy has a moderate size appearance.
