The galaxy presents a somewhat amorphous, rather than well-defined, structure. It's morphology appears to be more smooth than highly structured, with no obvious spiral arms or a distinct galactic bar visible. There seems to be a slight elongation, suggesting it is not perfectly spherical. The galaxy exhibits a color gradient, with a central brighter, slightly blue/green toned region which could indicate a concentration of younger, hotter stars or active galactic nuclei activity. The outer regions seem to be more red/orange. Patches of redder material suggest some dust lanes or regions of on-going star formation. The galaxy exhibits a mass upwards of 10^11 solar masses, with low star formation rates and a high degree of smoothness. There is a chance the galaxy might be experiencing a small merger event or minor disturbance, given its overall slightly disturbed appearance.
