The galaxy presents a largely featureless, smooth morphology, appearing nearly round in shape. The light is concentrated toward the center. There is a distinct, bright central bulge, with a yellow-orange hue, suggesting an older stellar population. The outer regions display a gradual decrease in luminosity, with a slightly bluer tinge, indicating the possible presence of younger stars, though star formation is likely low. No spiral arm structure or bar is discernible. There is no evidence of any major disturbances or ongoing merging events.
