The galaxy presents a somewhat disturbed morphology, possibly indicative of an interaction or recent merger event. It has a central, bright region that appears to be bulge-dominated. Diffuse, asymmetric extensions are observed extending outwards from this central bulge. These features display a mottled texture, with hints of star-forming regions and dust lanes. The overall color gradient suggests a relatively old stellar population, with a noticeable presence of ongoing star formation. Neutral hydrogen is detected, corresponding to the galaxy. The disk component is partially visible, but is disrupted and irregular in appearance.
