The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. There is a marked concentration of light towards the galactic center, which is consistent with the presence of a bulge. The color is moderately yellow to white, implying an older stellar population and relatively low levels of current star formation. There is no evidence of spiral arms, dust lanes, or significant morphological disturbances, although the object has some irregular edges to the galactic halo. The galaxy appears undisturbed, showing no signs of mergers or tidal interactions.
