The galaxy presents as a relatively smooth and compact structure. It exhibits a centrally concentrated light distribution, appearing elliptical or lenticular in shape, with no discernible spiral arms or bar features. The galaxy's color appears to be on the redder side, which suggests an older stellar population with a relatively low rate of on-going star formation. There is no obvious evidence of recent mergers or major disturbances in the galaxy's morphology. The object is neither perfectly round nor highly elongated, but appears somewhat in between these extremes. There appears to be little to no fine structure, such as dust lanes or tidal tails. The galaxy does not present a well-defined disk.
