The observed galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears concentrated toward the center, with a gradual decrease in intensity moving outward, suggesting an older stellar population. The overall color is somewhat redder, indicating a lower rate of star formation and a lack of prominent spiral arm structures. There appears to be a slight asymmetry, which could potentially be due to a minor gravitational interaction or disturbance. However, there is no significant evidence of major mergers or tidal tails. Based on these visual characteristics, the galaxy is most likely an elliptical or lenticular galaxy. 
