The observed galaxy presents a distinct disk-like morphology, viewed at an angle that indicates it is somewhere between face-on and slightly tilted. The galaxy exhibits prominent spiral arm structures. The galaxy also seems to have a large moderate bulge, and the galaxy has a bar. There is no apparent tidal disruption, no clear merging, and no major disturbances. The color distribution suggests a diverse stellar population, with a central concentration of older, redder stars and bluer regions associated with the spiral arms, likely indicating ongoing star formation.