The galaxy presents as a relatively smooth, elliptical structure. It exhibits a cigar-shaped morphology with a noticeably elongated profile. There is little evidence of significant disk-like structure or spiral arms. The central region appears brighter and more concentrated than the outer edges. There is no clear sign of recent major merger activity or significant tidal disturbances. The galaxy displays a generally homogenous light distribution with some subtle color variations. The core exhibits a yellow hue transitioning into blue fringes that might indicate areas of recent star formation. This may suggest a transition between a passive red-and-dead galaxy and a younger blue galaxy.
