The galaxy presents a generally smooth, rounded morphology. Its light is dominated by blue-white hues. A bright, concentrated central region, possibly the galactic nucleus, shows indications of active processes. A slight irregularity in the smooth light distribution may suggest either some disturbance or perhaps the early stages of a merging event, though more data would be necessary to confirm. The overall roundness indicates that it is likely an elliptical or lenticular galaxy, but the color suggests the presence of recent or ongoing star formation in parts of the galaxy.
