The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light profile appears relatively uniform, transitioning gradually from a bright, unresolved core to a fainter, more diffuse outer region. There is a slight ellipticity to the overall shape, deviating minimally from a perfectly circular form. No distinct spiral arms or bar structures are discernible. The color gradient exhibits a subtle trend, with the core appearing marginally bluer than the outer regions, suggesting potential ongoing star formation activity near the center. There is no strong evidence of tidal disturbances or interactions with other galaxies. 
