The galaxy presents a generally smooth, oval morphology, appearing to be an elliptical galaxy. There appears to be an apparent lack of strong spiral arm structures or significant dust lanes. The color gradient shows a brighter, more concentrated central region that is more yellow, suggesting an older stellar population. The outer regions appear somewhat bluer, hinting at the presence of younger stars, though not prominently. There may be some evidence of minor tidal disturbances, based on some slight asymmetry in the outer regions, but it is likely that the galaxy is in a relaxed state. The galaxy does not appear to be undergoing any major merging events. It appears to be a relatively massive system. Star formation is most likely low.
