The galaxy presents a predominantly smooth morphology, with a concentrated central bulge that emits strongly in the g, r, and z bands suggesting older stellar populations. The overall shape appears relatively round, showing minimal signs of elongation or distortion. There is some indication of a possible minor interaction or tidal disturbance, with a slight asymmetry in the outer regions that hints towards ongoing or recent accretion activity. The galaxy's color is generally yellowish-orange, but there is bluer star formation that may be occurring off to the side of the central bulge.
