This galaxy appears to exhibit a complex morphology. The primary component presents a relatively smooth light distribution suggesting an elliptical galaxy. It possesses a central bulge, with a moderately elliptical shape, displaying a gradual decrease in luminosity from the core outwards. There is evidence of a potential minor disturbance in the system. This disturbance appears in the form of a plume or tidal feature that could indicate a past or ongoing interaction with another galaxy. Further analysis would be necessary to confirm.
