The galaxy presents a predominantly smooth morphology. It appears largely featureless with a high degree of central concentration. There is a slight elongation. The light distribution indicates a generally elliptical shape. A subtle hint of asymmetry might suggest a minor disturbance within the galaxy or recent interaction with a smaller object, though this could also be an artifact. The color profile suggests an older stellar population. The redder hue is indicative of evolved stars. Overall, the galaxy is a relatively quiescent system without significant ongoing star formation. A possibility of a late stage merger or a recent interaction cannot be ruled out.
