The galaxy presents as a relatively smooth, elliptical-like system with a concentrated central bulge. The core exhibits a yellowish-white hue, suggesting an older stellar population. Surrounding the core, a faint, bluish-greenish disk or extended structure is present, possibly indicating some ongoing star formation. The galaxy displays a slight asymmetry, with the outer regions appearing more extended along one axis. There are no clear signs of major tidal disturbances or a recent merger event, although a minor interaction cannot be ruled out. The overall morphology suggests a system transitioning from a disk-dominated to a more spheroidal shape, with a moderate mass and low to moderate star formation rate.
