The galaxy presents a largely smooth, elliptical morphology, with a concentrated central bulge that emits strongly in the g, r, and z bands. The light distribution suggests a high degree of symmetry, with isophotes appearing roughly circular to moderately elliptical. There may be evidence of minor disturbances in the outer regions, potentially indicating interaction with nearby objects, or past merger events. The object is relatively large and has a high mass, exhibiting characteristics of a mature stellar population. Given its red color and apparent smooth texture, it likely has minimal on-going star formation.
