The galaxy presents a somewhat distorted morphology, potentially indicative of past or ongoing interaction. It has a dominant, relatively smooth central bulge with a golden hue, suggesting an older stellar population. Extending from this bulge is a fainter, bluer arm or tidal feature, displaying a region of more recent star formation. The overall shape appears elongated, deviating from a perfect elliptical form. The asymmetry and the presence of the arm/tidal feature suggest a system that is not entirely relaxed and may be undergoing some form of gravitational disturbance. There's also a slight suggestion of faint, diffuse light surrounding the main body of the galaxy, possibly representing an extended halo of stars.
