The galaxy presents an elongated, somewhat elliptical morphology. The central region exhibits a concentrated, bright yellowish hue, indicating a substantial population of older stars. Extending outward from the core, there is a diffuse, fainter disk. The color of the disk appears slightly bluer than the nucleus, suggesting the presence of younger stars, perhaps resulting from ongoing or recent star formation. The galaxy appears relatively undisturbed, displaying no obvious signs of major mergers or tidal interactions. Overall, it exhibits characteristics consistent with a disk galaxy exhibiting modest star formation and a significant spheroidal component.
