The galaxy presents as a somewhat inclined spiral, exhibiting a moderately bright central bulge. The bulge appears relatively smooth in texture and is of an elliptical shape. Faint spiral arms are visible extending from the central region, though their definition is indistinct. A slight asymmetry in the arm structure can be observed. The color gradient suggests a higher concentration of older stellar populations within the bulge, with a gradual transition to bluer hues in the outer regions of the disk. The overall light distribution implies a substantial stellar mass, with an estimated star formation rate that falls within the range typically seen in galaxies of this morphology at its estimated redshift. There is no obvious tidal distortion or evidence of a major merger event.
