The galaxy presents as a relatively smooth, elliptical object with an apparent cigar shape. The core region exhibits a concentrated, bright, yellow-orange hue, possibly indicating an older stellar population. The outer regions are dimmer and display a subtle greenish tint, which could suggest the presence of a younger stellar population or ionized gas. There is no clear evidence of spiral arm structures or major disturbances, which are characteristics typically associated with late-type galaxies. Faint diffuse light extends beyond the main body, implying a sizable halo or envelope of stars. The overall morphology suggests an evolved galaxy, possibly undergoing passive evolution.
