The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. Its light profile suggests an older stellar population, characterized by a yellowish-red hue. There is a distinct lack of blue light, indicating a limited amount of ongoing star formation. The galaxy shows no apparent spiral arms or prominent dust lanes. Its overall shape is mostly round, with only slight ellipticity. There is no evidence of any major merging activity or significant tidal disturbances. Based on its redshift, the galaxy is at a considerable distance and demonstrates a high stellar mass. The low star formation rate places it in the category of a quiescent or passive galaxy.
