This galaxy exhibits a moderately disturbed morphology. Its overall shape appears somewhat elliptical, but with noticeable asymmetries. The central region displays a bright, concentrated core, possibly indicating the presence of an active galactic nucleus. A faint, diffuse halo surrounds the core, extending outwards with irregular edges. Patches of blueish light, suggestive of younger stellar populations and ongoing star formation, are scattered throughout the galaxy's disk. Evidence of tidal features, potentially from an interaction or minor merger event, are visible as faint plumes or extensions emanating from the main body of the galaxy. Overall, the galaxy suggests a system undergoing or recently recovered from gravitational interactions, displaying a mix of old and young stellar populations with ongoing, albeit potentially low-level, star formation activity.
