The galaxy presents as a single, somewhat concentrated object. The morphology appears generally smooth and elliptical with a high degree of central concentration. The object appears fairly round. The color profile trends towards redder hues, with a luminous yellow core, suggesting an older stellar population and potentially a lack of significant ongoing star formation. There is no obvious indication of spiral arms or a disk structure. There is no obvious indication of any major merger events. The size seems to be of intermediate scale, neither exceptionally large nor particularly compact. 
