The galaxy presents as a generally smooth, elliptical object, with a concentrated central bulge. The color appears to be predominantly yellowish-orange. It exhibits a relatively high degree of roundness, with no apparent spiral arm structure or prominent dust lanes visible in this imaging. There is no evidence of a major ongoing merger, though some minor asymmetry may be present, suggesting a possible past interaction or minor disturbance. The galaxy's overall structure seems undisturbed, exhibiting a degree of central concentration suggesting a potentially evolved stellar population.
