The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The shape appears to be neither perfectly round nor highly elongated, leaning towards an intermediate form. There is a hint of a disk-like structure, though the smooth component dominates. Faint tidal tails are visible, suggesting a potential history of interaction with another galaxy. The core region displays a pronounced yellowish hue, possibly indicating an older stellar population, while the outer regions appear slightly bluer, hinting at ongoing star formation activity. The overall color gradient suggests a radial variation in stellar populations, with older stars concentrated towards the center and younger stars more dispersed in the outskirts. There's an indication of a minor disturbance or interaction on one side of the galaxy. Overall, this galaxy appears to be a transitioning system, potentially evolving from a disk-dominated to a more spheroidal form, with evidence of recent or ongoing star formation activity.
