The galaxy presents as an elliptical morphology. It appears relatively smooth, with no immediately discernible spiral arm structure or prominent dust lanes. The central region exhibits a concentrated luminosity, indicative of a substantial galactic nucleus. Coloration is predominantly yellow, suggesting an older stellar population with a diminished rate of star formation. There is a slight hint of a potential tidal feature or minor disturbance at one edge, meriting further investigation to determine if an interaction has occurred. The roundness of the galaxy indicates that the galaxy is not viewed edge-on. 
