The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its morphology is dominated by a nearly spherical shape, showing minimal signs of a disk structure or spiral arms. The core exhibits a bright, yellowish-white hue, indicative of an older stellar population. The outer regions display a gradual decrease in surface brightness, with a faint blue tinge that could possibly be a faint sign of limited ongoing star formation. There are no signs of any major disturbances, tidal tails, or ongoing mergers, with possibly a minor disturbance on the left. The galaxy appears to be relatively isolated in its environment.
