The object appears to be a spiral galaxy viewed at a slight inclination, exhibiting a distinct disk-like structure. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer spiral arms extend outwards from the bulge, although their definition is somewhat blurred. These arms imply ongoing star formation within the disk. The overall morphology suggests a galaxy with a moderately active rate of star formation, likely in the later stages of its evolution. There appears to be little to no evidence of a significant ongoing merger or major tidal disturbance. The dust lanes are not apparent, but this is due to the galaxy being viewed at such a great distance. 
