The galaxy presents an elliptical morphology, appearing largely smooth and featureless in this image. The central region exhibits a concentration of light, appearing bright and yellowish-orange in color, suggesting an older stellar population. The outer regions appear less luminous, with hints of a disk-like structure or some form of extended features. There is some evidence of potential disturbances, possibly from a past or ongoing minor merger event, although the dominant impression is one of a relatively settled system. The galaxy shows a redshift, indicating it is receding from us. There are no obvious spiral arms or strong dust lanes visible. Overall, the galaxy seems to be a massive galaxy with a relatively low star formation rate.
