The galaxy presents as a primarily smooth, elliptical or spheroidal structure. The light profile appears centrally concentrated with a bright, yellowish core, possibly indicative of an older stellar population. There is little evidence of spiral arms or significant dust lanes. The overall shape is close to circular, showing minimal elongation. The galaxy appears to be isolated, with no obvious signs of ongoing major mergers or tidal disturbances. Faint blue hues in the outer regions may indicate regions of lower level star formation. 
