The galaxy presents as a disk-type system, viewed at an intermediate angle. A central bulge region appears present, though not dominant in size relative to the disk. Subtle hints of spiral arm structures emanate from the central region. Blue color suggests moderate on-going star formation. The system exhibits some level of disturbance, with irregular features visible in the disk structure, suggestive of a possible interaction or merger event, but no defined companion object is visible. There is no strong bar structure.