The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellowish-white hue, possibly indicating an older stellar population and a lower rate of on-going star formation within the nucleus. The galaxy gradually fades outwards from its central region, with the outer regions appearing less luminous and exhibiting a slightly bluer tint. There is no apparent disk structure or spiral arm features visible. The galaxy appears relatively undisturbed with no major signs of tidal interactions or ongoing mergers. There is a subtle color gradient, suggesting that the stellar populations may vary in age across the galaxy, with the outer regions potentially containing a younger stellar population. The overall roundness of the galaxy indicates it is likely an elliptical galaxy, although subtle asymmetries may indicate some level of past interaction or accretion event.
