The galaxy appears to be a spiral type, exhibiting a relatively well-defined disk structure. Two prominent spiral arms are visible, extending from a central bulge. The arms display a moderate degree of winding, neither tightly wound nor particularly loose. There is some suggestion of flocculence, with segments of arms appearing disjointed. 

The central bulge is noticeable, occupying a substantial fraction of the galaxy's overall size and luminosity. It displays a color gradient, shifting to redder hues towards its center, suggesting an older stellar population concentrated towards the core.

The disk component shows a mix of blue and yellow hues, potentially indicating active star formation within the spiral arms alongside a more evolved stellar population. The overall color suggests a moderate redshift, placing it at a significant cosmological distance. There is no indication of a strong bar structure. No signs of significant tidal disturbances or ongoing major mergers are immediately apparent, although subtle irregularities in the arm structure might hint at minor gravitational interactions or past accretion events.
