The galaxy presents a relatively smooth morphology, with a discernible central bulge. The overall shape appears moderately round, although not perfectly spherical. There is faint evidence of spiral arms or other disk-like features, but any structure is poorly defined. The galaxy does not appear to be undergoing any major merging activity, though minor disturbances cannot be fully ruled out. Color gradients are present, with a bluer hue concentrated in the central region, possibly indicating recent star formation, while the outer regions exhibit a redder tone.
