The galaxy presents as a roughly elliptical or possibly a spiral galaxy viewed at a significant inclination, showing a central bulge and a surrounding, somewhat diffuse disk. The central bulge exhibits a yellowish-white hue, suggesting a population of older stars. The disk appears bluer, indicative of ongoing star formation and a younger stellar population. There is some indication of slight asymmetry and possible disturbance in the outer disk, though this could also be artifacts of the image quality. The overall structure seems to lean more towards a disk galaxy than a spheroid one.
