The galaxy presents as a predominantly smooth, elliptical object. The morphology is generally round, showing minimal deviation from a circular shape. It is relatively compact, appearing to lack significant spiral arms or disk-like features. The light distribution is concentrated towards the center, indicative of a prominent bulge. Color analysis suggests a population of older stars and potentially low levels of on-going star formation. There is no strong evidence of any major ongoing merger events or significant tidal disturbances affecting the overall structure of the galaxy.
