The galaxy presents a somewhat amorphous morphology, appearing neither distinctly elliptical nor spiral. It is centrally concentrated with a bright core region, indicating the likely presence of a supermassive black hole. The overall color is moderately blue, suggesting at least some ongoing star formation, though the rate is unlikely to be exceptionally high. The light distribution suggests a relatively smooth profile, with minimal evidence of strong spiral arm structures or prominent dust lanes. The shape deviates slightly from perfectly circular, displaying a subtle elongation. There is possible evidence of minor disturbances in the galactic structure, which could indicate a past or ongoing minor merger event.
