The galaxy presents a distinct spiral morphology. Evident spiral arms emanate from a central bulge region. The winding of the spiral arms appears to be of an intermediate nature, neither tightly wound nor loosely defined. Two prominent spiral arms are observable. The bulge component appears moderate in size relative to the overall galactic disk. There is no apparent presence of a strong bar structure bisecting the bulge region. The disk is inclined at an angle to our line of sight. The morphology indicates a possibility of a minor interaction or disturbance with a nearby object.