The galaxy presents as a spiral type, oriented roughly face-on. Two prominent spiral arms are clearly visible, winding moderately outward from a central bulge. A bar structure appears to extend through the central region, though it seems to be somewhat weak in definition. The bulge size appears to be moderate relative to the overall disk. The disk itself exhibits a blueish hue, indicative of active star formation. The spiral arms show irregularities and some flocculence, with variations in color suggesting varying stellar populations and dust content. There is no obvious sign of a major merger, but some minor disturbances in the outer disk cannot be ruled out. The galaxy appears to be at an intermediate redshift, suggesting a considerable distance.
