The galaxy presents as an elliptical morphology, with a high degree of smoothness. It exhibits an overall circular shape, showing little to no deviation towards a cigar-like appearance. There is no clear indication of any major merger events or significant disturbances in its structure. The stellar mass is estimated to be significant, around 10^9.6 solar masses, with star formation activity appearing to be largely quenched, as indicated by the low star formation rate. The galaxy's color suggests it is composed primarily of older stellar populations.
