The galaxy presents a somewhat elongated morphology, appearing as a disturbed system. The main body exhibits a relatively smooth, though not perfectly uniform, light distribution. The central region is brighter and appears more concentrated. Fainter, diffuse features extend outwards, possibly indicative of tidal tails or disturbed spiral arms. There is a hint of blueish coloration in the central region, potentially indicating the presence of younger stars. The overall color suggests a population of intermediate-age stars, with ongoing, but perhaps not exceptionally vigorous, star formation. Evidence of possible interaction or merging activity is suggested by the irregular shape and diffuse extensions. There also appears to be evidence of dust obscuring certain regions of the galaxy.
