The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting an overall elliptical shape. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is little evidence of spiral arms or significant dust lanes. The galaxy's color index suggests a population of older stars, exhibiting a reddish-yellow hue. The galaxy shows some evidence of minor disturbances, which could be indicative of a past or ongoing interaction with another galaxy. Based on the morphology, the galaxy is likely a relatively evolved system with a low star formation rate.
