The galaxy presents a largely smooth and rounded morphology, lacking prominent spiral arms or a distinct bar structure. Its color is primarily a yellowish-orange hue, indicative of an older stellar population with fewer young, massive stars. The light appears concentrated towards the center, suggesting a prominent bulge or a centrally located supermassive black hole that is not actively accreting. There are only the slightest irregularities in the light distribution and no sign of tidal tails or any major disturbance.
