The galaxy exhibits a prominent spiral structure, characterized by two well-defined arms emanating from a central region. These spiral arms display a moderate winding, neither tightly wound nor loosely spread, indicating an intermediate stage of spiral arm development. The arms themselves appear somewhat flocculent, exhibiting patchy regions of enhanced brightness indicative of active star formation. The central bulge appears moderate in size relative to the overall galactic disk. There is no evidence of a strong bar structure bisecting the galactic center; a weak bar may exist but it cannot be confirmed by looking at the image. The overall color of the galaxy suggests a diverse stellar population, with bluer regions likely corresponding to younger stars and redder regions indicating older stellar populations. The galaxy's morphology shows no signs of a major merger event, though minor disturbances cannot be entirely ruled out.
