The galaxy presents as a fairly smooth, centrally concentrated object. Its morphology appears to be elliptical or lenticular, displaying a generally rounded shape. There is a dominant central bulge that gradually diffuses outwards into a less defined halo. A very faint hint of a disk structure is barely visible at the center. There are no signs of significant spiral arms or prominent dust lanes. The galaxy displays a blueish color, suggesting the presence of younger stellar populations, even though the star formation rate appears to be relatively low. There is no obvious evidence of an ongoing merger event or major tidal disturbances. The galaxy appears to be relatively undisturbed.
