The galaxy presents as a single, relatively smooth object with a high degree of central concentration. Its overall shape appears round, lacking any obvious disk-like structure or elongated features. The galaxy's light profile suggests a gradual decrease in luminosity from the center outwards. There is no clear evidence of spiral arms, bar structures, or prominent dust lanes. The color appears somewhat redder compared to other objects in the field. There is no clear evidence of any ongoing major merger events or significant tidal disturbances. The galaxy appears to be relatively isolated, without any bright or large companions nearby. Based on its apparent smoothness and round shape, the galaxy is likely an elliptical. 
