The galaxy exhibits a generally smooth morphology, although the presence of subtle features cannot be entirely ruled out. The light distribution appears centrally concentrated, suggesting a possible spheroidal or elliptical shape. Color gradients are apparent, with a bluer hue observed in the outer regions and a redder color towards the center. This could be indicative of varying stellar populations or dust content within the galaxy. There may be slight disturbances or asymmetry within the light profile, and a faint, extended halo seems to be visible at a distance from the main body of the galaxy.
