The galaxy presents as a relatively smooth, elongated structure. Its light is concentrated towards the center, which appears as a bright, unresolved bulge. The overall color is somewhat red-shifted. The galaxy seems to be transitioning from a disk galaxy to a smoother, more spheroidal shape. The light distribution appears somewhat irregular, indicative of possible minor gravitational interactions. There may be slight disturbances in the disk. Evidence of a merger is slight, with the overall structure remaining relatively undisturbed. The galaxy is relatively massive with mild star formation activity.
