The galaxy presents an elliptical morphology, appearing largely smooth and relatively featureless. The light distribution is centrally concentrated with a gradual decrease in luminosity towards the outer regions, which suggests an older stellar population. There is a slight elongation but overall, it appears mostly rounded. There is no apparent spiral structure or dust lanes visible within the galaxy. There's no evidence of strong tidal features suggesting a recent major merger. The galaxy exhibits a moderately low star formation rate. Overall, this galaxy appears to be an elliptical galaxy undergoing passive evolution.
