The galaxy presents a largely smooth and rounded morphology. It exhibits a concentrated central bulge that gradually fades into a less defined outer region. There is a subtle hint of a disk-like structure, although any spiral arms or distinct features are either absent or below the resolution threshold. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal distortions. Its color is primarily a redder hue, suggesting an older stellar population and/or a significant amount of dust obscuration. Faint hints of bluer regions may indicate pockets of younger star formation, although these are not prominent. Overall, the galaxy seems to be a relatively quiescent system with an evolved stellar population, potentially classified as an early-type spiral or lenticular galaxy.
