The galaxy presents as a spiral type, observed at a moderate redshift. It displays a prominent bulge region, surrounded by a fainter, more diffuse disk.

The spiral arms are tightly wound around the central bulge. They appear somewhat fragmented, with a high degree of symmetry and at least two arms originating from the bar region, although the definition of the arm count is obscured by the image quality. There is no evidence of significant tidal disruption, although there is a slight distortion to the left of the galaxy.

The bulge exhibits a yellowish hue, suggestive of an older stellar population. The disk shows bluer regions, indicating ongoing star formation. Overall, the galaxy appears to be in a relatively quiescent state, showing low star formation.
